Upload
chememeera
View
3.510
Download
4
Embed Size (px)
Citation preview
1
Chem 425- Mass SpectrometryTuesday and Thursday: 10am – 11:20am, C2-361
Richard W. Smith, [email protected]
C2-264 (office) / C2-267 (lab)UW Mass Spectrometry Facility
Course TA: Jonathan [email protected]
Office Hour: Friday, 12:30pm-1:30pm, C2-269B
2
Course Overview• 1. Introduction
• 2. History
• 3. Electron Ionization– The mass spectrometer and mass calibration– Electron Ionization (EI)
• Fragmentation• QET• Elemental composition, isotopic species, mass resolution, accurate mass, z>1,
rings plus double bonds, nitrogen rule• Interpretation of EI mass spectra
• 4. Chemical Ionization (CI and DCI)– Ion formation– Thermochemical considerations and reagent systems– Negative ion formation
3
Course Overview cont• 5. Field Ionization and Field Desorption (FI and FD)
• 6. Particle Bombardment– FAB, LSIMS and 252Cf
• 7. Laser Desorption Ionization and Matrix Assisted Laser DesorptionIonization (LDI and MALDI)
• 8. Inductively Coupled Plasma (ICP)
• 9. Atmospheric Pressure Ionization (API)– Electrospray (ESI)– Atmospheric Pressure Chemical Ionization (APCI)– Atmospheric Pressure Photo-Ionization (APPI)
4
Course Overview cont• 10. Mass Separation
– Magnetic and electrostatic fields (B and E)– Quadrupoles (Q and QQQ)– 3D Quadrupole Ion Trap (QIT)– 2D linear Ion Trap– Time of Flight (Tof)– Fourier Transform Ion Cyclotron Resonance (FTICR)
• 11. Hyphenation in Mass Spectrometry– Gas Chromatography – Mass Spectrometry (GC-MS)– Liquid Chromatography – Mass Spectrometry (LC-MS)
• Interfaces– MS-MS and MSn - Tandem Mass Spectrometry
• Collision Induced Dissociation (CID)• BE, QQQ, 3D QIT, 2D QIT, QTof……
5
Course Overview cont
• 12. Quantitation– Primarily with QQQ in MRM/SRM mode
• 13. Ion detection and Focusing– Faraday cup, Electron multiplier, multichannel plate and photomultiplier
• 14. Summary
6
Course Overview cont• 70 minute mid-term exam during class (Thursday, February 28th) –
25%• 150 minute final exam (to be scheduled) – 55%• 10 Weekly Quizzes – total of 10%. Held at the end of class starting on
Tuesday, Jan 15th (~10min)– 10 questions/quiz– 7 to 10 correct answers 1 mark– 3 to 6 correct answers 0.5 mark– 0 to 2 correct answers 0 mark
• 12 minute seminar – 10%. Held weekly at the end of class starting on Thursday, Jan 17
– Teams of 2 prepare and present the material
7
Course CalendarJanuary 2008
24 class sessions: Tuesday and Thursday – 10am to 11:20am in C2-361
31Sem 3
6. Particle Bombardment
3029Quiz 3
5. FI and FD
2827
262524Sem 24. CI
2322Quiz 24. CI
2120
191817Sem 13. EI
1615Quiz 13. EI
1413
1211103. EI
981. Introduction2. History
76
54321
SatFriThursWedTuesMonSun
8
Course Calendar
February 2008
2928Mid-Term
2726Quiz 69. API
2524
23222120191817
161514Sem 59. API
1312Quiz 59. API
1110
987Sem 48. ICP
65Quiz 47. LDI & MALDI
43
21
SatFriThursWedTuesMonSun
Reading Week
9
Course Calendar
March 2008
3130
292827Quiz 10
12. Quantitation
2625Sem 9
11. Hyphenation
2423
222120Quiz 9
11. Hyphenation
1918Sem 8
11. Hyphenation
1716
151413Quiz 8
11. Hyphenation
1211Sem 7
10. Mass Sep
109
876Quiz 7
10. Mass Sep
54Sem 6
10. Mass Sep
32
1
SatFriThursWedTuesMonSun
10
Course CalendarApril 2008
30292827
26252423222120
19181716151413
1211109876
543Sem 11 &1214. SummaryQ and A
21Sem 10
13. Ion Focusingand Detection
SatFriThursWedTuesMonSun
ExamsStart
11
ResourcesText Books
• Mass Spectrometry – A Textbook (on 1 hour hold at Davis Library)
Jurgen H. Gross - Springer 2004 – QD96M3G76
• Mass Spectrometry: A Foundation Course
K. Downard – Royal Society of Chemistry 2004 – QD96M3D69X2004
• Chemical Ionization Mass Spectrometry – 2nd edition
Alex G. Harrison – CRC Press 1992 – QD96M3H371992
• Interpretation of Mass Spectra
Fred W. McLafferty – University Science Books
Database website• NIST Library of EI Mass Spectra:
http://webbook.nist.gov/chemistry/name-ser.html
12
Journals:
• Biomedical and Environmental Mass Spectrometry / Biological Mass
Spectrometry
• International Journal of Mass Spectrometry
• Journal of the American Society For Mass Spectrometry
• Mass Spectrometry Reviews
• Journal of Mass Spectrometry
• Rapid Communications in Mass Spectrometry
Resources
1
History• 1913: J. J. Thomson – parabola spectrograph
– Detection of the neon isotopes 20 and 22
– Parallel electric and magnetic field
– Detection on photoplate
Photoplate detector
Gas Discharge ion source
Focusing
Mass separation usingmagnetic and electric fields
+ve and -ve ionsrecordedsimultaneously!
+
-
2
J. J. Thomson: First Mass Spectrum of 20Ne and 22Ne
Modern measurements of 20Ne:22Ne ~ 10:1
3
History• 1918 – 1920: Dempster and Aston (Nobel prize in 1922)
– Focussing of ions– Higher resolution (≈ 600)– tandem electric and magnetic field– Allowed the detection of 21Ne (0.3% abundance)
4
• Late teens to early 30‘s, MS primarily used for isotopic analyis of the stable elements
• 1934: J. Mattauch and R. Herzog (Nobel prize)– Double focusing instruments > resolution 6500
• 1936: Secondary Ion Mass Spectrometry introduced
• 1940: Westinghouse Electric begins development of a portable MS for commercial sale
• 1942: E.O. Lawrence develops the “Calutron“ prep scale MS for separation of uranium isoptopes – 235U
• 1943: CEC installs 1st commercial MS at the Atlantic Refining Company
• 1945: CEC introduces 1st analogue computer for data analysis
History
5
History
• 1946 -1947: 1st description of time-of-flight MS, Metropolitan Vickers and General Electric begins manufacturing MS
• 1948: ICR MS “Omegatron“ is developed
• 1952: 1st A/D converter for data aquisition (CEC)
• 1953: W. Paul → Quadrupole mass spectrometer and ion trap detectors – Nobel prize in 1989.
• 1954: 1st high resolution MS developed at Imperial Chemical Industries (ICI)
• 1956: PA determinations made by MS, McClafferty rearrangment described, steroids 1st analyzed by MS
6
History• 1957: GC/MS 1st demonstrated at Phillip Morris
• 1958: CEC introduces the 1st digitizer. Bendix TOFMS introduced
• 1959: peptides and oligonucleotides sequeunced at MIT
• 1960: Bendix introduces 1st direct insertion probe– CEC introduces 1st high res double focusing MS
• 1966: Tandem MS for ion-molecule studies is developed– Chemical Ionization is developed at ESSO (Munson and Field)
• 1968: Electrospray Ionization introduced at Northwestern U for studying macromolecules. Computer library searching used for identification of unknown compounds
7
• 1969: 1st GC/MS with integrated computer introduced
• 1971: relectron time-of-flight develpoed in Lenningrad
• 1974: M.B. Comisarow, A.C. Marshall – FT-MS. APCI interface is developed for LCMS
• 1975: mass spectrometers are placed on the Viking Mars missions
• 1979: Ion evaporation model developed (ESI)
• 1980: ICPMS is developed at Iowa State U. 1st commercial QQQs introduced.
• 1981: FAB introduced.
• 1983: A.L. Yergey, M.L. Vestal – Thermospray interface for LCMS announced.
History
8
• 1984: Yamashita and Fenn – Electrospray (Nobel prize, 2002). 1st
commercial ion trap is introduced. Particle Beam interface developed at GIT.
• 1986: LC interfaced to MS with pneumaticaly assisted ESI.
• 1988: Karas and Hillenkamp – MALDI
• 1994: Micro- and nano- ESI are introduced
• In the past 10 years a wide variety of hybrid instruments have been introduced along with great improvements in instrument capabilities and sensitivity (attamole)
History
1
The Mass Spectrometric Process
Ion source Mass Analyzer(s) DetectorSample Introduction
Gas or condensedphase sample +
Some form ofionization
Ions
Separates ions basedon their m/z value
Indirectdetection
*Field free regionwith ion focusing
* *
Integrated with some degree of computer control
2
The Mass Spectrometer• Sample Introduction
• Batch - direct insertion probe, desorption probe, heated inlet, infusion
• Chromatographic – GC or LC (SFC)
• All Ion sources produce either
• Odd electron ions eg M+. (EI, charge exchange CI)• Even electron ions eg [M+H]+, [M-H]- and/or adducts
[M+Na]+
(CI, FAB/SIMS, ESI, APCI, APPI)• Stability of these ions determines the observed mass
spectrum
3
The Mass Spectrometer• All Mass Analyzers
• Separate ions according to their mass/charge ratio (m/z)
• This separation is accomplished in a variety of fashions eg by momentum (BE/EB), time of flight (Tof), selective transmission employing Rf and DC voltages (Q and IT), frequency of motion (FTICR)
• MS/MS and MSn
• Continuous beam (Q, BE/EB) and pulsed beam (IT, Tof, FTICR)
• All Detectors• Conversion of +ve and –ve ions to 2o electrons or photons• Indirect detection
• Computer employed for instrument control, data acquisition and processing
4
JEOL HX110 Double Focusing Mass Spectrometer (EB)
Detector
Magnet
Source andSample Introduction
TuningConsole
ESA
5
Benchtop Quadrupole GC/MS system
Courtesy of Agilent
GCMS
6
Ion Types• Molecular ions: [M]+•, [M]-• are ions that arrive intact at the
detector– Stable – k < 105s-1
• Fragment ions: [F]+ formed in the source by direct bond cleavage or rearrangement– Unstable k > 106s-1
• Metastable ions, m* are ions that fragment outside the ion source but before they arrive at the detector– 105s-1 < k < 106s-1
7
Ion Types
M+.
Fragment ions
Metastable ion
M+. and fragment ions~0.3Da wideMetastable ion~3Da wide!
8
Ion Types• Odd electron (such as [M]+•) and even electron ions (such as
[M+H]+)
• Quasi-molecular ions, e.g. [M+H]+, [M-H]-, [M+NH4]+, [M+Na]+, [M+Cl]- ……..
• Cluster ions, [2M+H]+, (proton bound dimer)
• Isobaric ions (same nominal mass)
• Isotopic species
9
Mass Calibration
• All mass spectrometers make ions, pass them through a region where they are separated according to their m/z ratio and finally detected
• A mass calibration must be performed in order to convert arrival times of ions at the detector into a m/z value
• This is achieved by introducing a reference compound(s) into the source who’s masses are known and then comparing this uncalibrated mass spectrum with a reference spectrum of the same compound(s). The patterns are matched and the data system then can, in real time, convert arrival times into m/z values.
• Reference compounds are many and varied eg PFK, PEG, CsI and other clusters such as phosphoric acid. The compound(s) chosen will depend upon the ionization mode employed.
10
Mass Calibration
• Perfluorkerosene (PFK) with the JEOL HX110
Uncalibrated Calibrated
62.3
344.6
493.1
69.0
380.94
542.9
Software algorithm
Uncalibrated ΔM at m/z 380.97 = 36.3Da Calibrated ΔM at m/z 380.97 = 0.03Da
11
Electron Ionization – The Source
Samplein
S
N
S
N
Trap
Focus plates
magnet
Ion beam out -M+. and fragment
ions
Source block
Filament
e-
Repeller
12
• Source operates at high vacuum (10-6 mbar) and high temp (~200oC)
• Electrons are produced by heating a filament with a few amps ie thermionic emission from a hot wire (rhenium or tungsten)
• They are focused onto the trap using a magnetic field and voltage - usually 70V (can be changed) therefore e- are said to have 70eV translational energy
• Trap: Collects the electrons on the far side of the source. Usually the trap current is set and the electronic circuitry adjusts the filament emission to maintain this value
• Repeller: +ve relative to the source, pushes the +ve ions formed toward and out the exit slit where they are further accelerated into the mass analyzer region
Electron Ionization
13
• Magnetic field causes e- to spiral increasing the chance of an interaction with the sample species – higher sensitivity
• Sample is introduced and must be volatilized before ionization can occur – iedilute gas phase unimolecularprocesses (same for EI and CI)
Electron Ionization
14
EI of Methyl Stearate at 70eV
M+.
O
O
Mwt=298.5095Monoisotopic mass=298.2872
15
• We need to understand the processes involved if we hope to use MS as a structural elucidation tool!
• Ionization
• Isotopic distribution
• Accurate mass
• Fragmentation
Electron Ionization
16
Ionization
• one of the most common forms of ionization
AB + e- AB+. + e- + e-
1o 1o 2o (slow)
A+ + B. etc
ΔHf (AB+.) = IP + ΔHf (AB)
IP is the ionization potential of AB ie the energy required to remove one electron
• note that radical cations (M+.) are initially formed
17
Ionization
• the term electron “impact” should be avoided as the electron does not impact the molecule
• 70 eV electrons have a deBroglie wavelength associated with them of about 1.4Angstrom which is on the order of a bond length. The interaction of the electron “wave” with the molecule causes a disturbance which causes excitation or ionization of the molecule
• Removal of the e- from a molecule can be considered to occur at:σ-bond < π-bond < free electron pair
18
Probability of ionization as a function of electron energy
• Maximum ionization efficiency of organic ions at 20 – 50 eV• every species has it‘s own curve depending on it‘s ionization cross section • Excess energy ( ~ 1 – 8 eV) can lead to substantial fragmentation
19
Electron Energy
• some of the energy of the electron goes into ionizing the molecule (~7-12 eV). There is still more than enough energy available to cause extensive fragmentation of molecules - typical bond strengths are 1 – 4 eV.
• The electron energy chosen must be higher than the ionization potential (IP) of the compound
• the higher the electron energy, the more energy there is available for fragmentation and therefore a higher degree of fragmentation is usually observed.
EI spectra of β-lactam using 70 and 15 eV electrons. Note the intensity scale.
20
Ionization
• The ionization potential (IP), is the minimum energy required to remove an electron from a species. The ionization cross section (σ) is a measure of the relative ease of ionization of a molecule. In general, this is proportional to the polarizability of the molecule.
• Polarizability is the relative tendency of the electron cloud of an atom to be distorted from its normal shape by the presence of a nearby external electric field
16.38.14-C10H8
10.39.2416.9C6H6
11.910.1322.3C6H14
6.3010.9411.1C3H8
4.4711.528.35C2H6
2.5912.614.30CH4
4.0412.137.31Xe2.4814.005.29Kr
1.6415.763.52Ar0.4021.560.62Ne0.2124.590.38He
Polarizability(10-24cm3)
IP (eV)
σ / A2Molecule
21
• For sufficiently energetic electrons, ionization may be accompanied by bond cleavage:
• Most of the energy exchanged creates electronic excitation (along with ionization). Almost no M+. ions will be in the vibrational ground state. “Some” of these vibrationally excited ions may be above the dissociation energy level
• The appearance energy (AE) of A+ from AB is defined as the minimum electron energy at which A+ is formed from AB. AE measurements are very useful for determining standard heats of formation however requires specialized instrumentation.
Appearance Energy (AE)
AB + e- → A+ + B + 2e-
AE = ΔHf (A+) + ΔHf (B) – ΔHf (AB)
22
Appearance Energy (AE)• For example: the appearance energy of CH2OH2
+ by dissociativeionization of HOCH2CH2OH (ethylene glycol), also producing neutral formaldehyde (CH2O) was found to be 11.42 eV (JACS 1982, 104, 2931). What is the heat of formation of CH2OH2
+ given that the heats of formation of ethylene glycol and formaldehyde are –387.6 and –108.7 kJ mol-1, respectively?
HOCH2CH2OH CH2OH2+ + CH2O
1eV=96.485 kJ mol-1Therefore 11.42 eV = 1102 kJ mol-1
AE = 11.42eV
23
Appearance Energy (AE)
AE = ΔHf (CH2OH2+) + ΔHf (CH2O) – ΔHf (HOCH2CH2OH)
or
ΔHf (CH2OH2+) = AE - ΔHf (CH2O) + ΔHf (HOCH2CH2OH)
ΔHf (CH2OH2+) = (1102 + 108.7 – 387.6) kJmol-1
= 823 kJmol-1
In fact, CH2OH2+ has been determined to be approximately
20 kJ mol-1 lower in energy than its conventional isomer CH3OH+ (ΔHf = 844 kJmol-1).
24
Fragmentation in EI
• Both simple bond cleavages as well as complex rearrangements may take place after EIie. simple bond cleavage, t-butyl chloride:
C(CH3)3Cl +e- C(CH3)3+ +Cl. +2e-
25
Fragmentation in EIie complex rearrangement (McLafferty Rearrangement)
McLafferty Rearrangement: any fragmentation that can be described as a transfer of a γ-hydrogen to a double bonded atom through a six-memberedtransition state with β-cleavage. Occurs in saturated aldehydes, ketones and carboxylic acidsDistonic Radical Cation: a radical cation in which the charge and radical sites areseparated
OH
.+CH2
CH2+
OH+
CCH3CH2
.
O
+ e- C3H6O+ + C2H4 + 2e-
2-pentanone
distonic radical cation
26
Fragmentation in EIStevenson’s Rule:
AB+ e- A+ + B. + 2e-
or A. + B+ + 2e-
For simple cleavage, the species of lower ionization energy will give the more abundant ion. Therefore:
If IE(A) < IE(B) then IA+ > IB+
EI of methanol
CH3+
IP=9.84eV OH+
IP=13eV
32
29
31
27
EI of acetone, (CH3)2CO
M+.
m/z 58
43
CH3+
IP=9.84eV
CH3CO+
IP=7eV
28
• A theoretical approach to describe the unimolecular decomposition of ions
• In most mass spectrometers, processes occur in the highly diluted gas phase therefore bimolecular reactions are rare
• isolated ions are not in thermal equilibrium with their surroundings and can only internally redistribute energy by dissociation or isomerization (rearrangement)
• The rate constant (k) of a unimolecular reaction is strongly influenced by the excess energy (Eex) of the reactants in the transition state
• Removal of an electron can be considered to occur at a σ-bond, π-bond or at a free electron pair
• For charge localization: free electron pair > π-bond > σ-bond and this is reflected in IE’s
Quasi-Equilibrium Theory (QET)
29
Ionization is very fast therefore termed to be a vertical ionization process.
Vertical Transitions
Dissociation coordinate
Energy
r0 r1
M
M+. stable
M.+ A+ + B.
IE
dissociationenergy
30
• EI occurs very fast ~ 10-16s and is a vertical process (Franck-Condon principle)
• The probability of a particular vertical transition from the neutral to a certain vibrational level is described by the Franck-Condon factors.
• The larger r1 compared to r0, the more probable will be the generation of ions excited even above their dissociation level
• Ionization tends to cause weakening of the bonding (bond lengthening) in the ion compared to it’s precursor neutral
• The shape of the potential energy surface will also influence the ions fate
Take Away Messages from QET
31
The elemental composition:
• The use of isotope peaks• High resolution for accurate mass determinations• Rings + Double Bonds
• double bond equivalents (DBE)
Interpretation of EI spectra:Elemental Composition
32
Some Common Isotopic Species
Element Type is sometimes termed X, X+1, X+2 etc
33
Isotopic Classification of the Elements
Some Definitions:
• Atomic number specifies the number of protons in the nucleus eg C is element 6 6C
• Atoms with the same atomic number but with different number of neutrons are termed isotopes eg 17Cl 35Cl and 37Cl (3:1)
• The mass number is the sum of protons and neutrons in an atomcan be confusing for example both 18Ar and 20Ca have a mass number of 40
• Elements are classified as: A 19F, 31P, 127IA+1 12C and 13CA+2 35Cl and 37ClA-1 6Li and 7Lipolyisotopic Sn 10 isotopes
34
Isotopic Distributions
Calculation of the abundance ratios of isotopic peaks of molecules containing two isotopes, where the isotope natural abundances are given as a and b and n is the number of this species in the molecule:
(a + b)n = an +nan-1b + n(n-1)an-2b2/(2!) + n(n-1)(n-2) an-3b3/(3!) + …. (binominal equation)
e.g. if n = 2:(a+b)² = a² + 2ab + b²
For two Cl atoms where a = 100 (35Cl) and b = 32 (37Cl):
100² + 2•100•32 + 32² = 100 : 64 : 10
Likewise if n=3: a3 + 3a2b +3ab2 + b3
and if n=4: a4 + 4a3b + 6a2b2 + 4ab3 +b4
35
mass12 13
%
0
100
mass119 120 121
%
0
100
mass1199 1200 1201 1202 1203 1204 1205
%
0
100
mass31 32 33 34 35
%
0
100
mass63 64 65 66
%
0
100
mass95 96 97 98 99
%
0
100
27 28 29 30 31mass0
100
%
55 56 57 58mass0
100
%
82 83 84 85 86 87mass0
100
%
18 19 20 21mass0
100
%
188 189 190 191mass0
100
%
Common Isotopic Distributions
C1 C10 C100 S1S2 S3
Si1 Si2 Si3 F1F10
36
Common Isotopic Distributions
34 35 36 37 38mass0
100
%
68 69 70 71 72 73 74 75mass0
100
%
103 104 105 106 107 108 109 110 111 112mass0
100
%
139 140 141 142 143 144 145 146mass0
100
%
78 79 80 81 82mass0
100
%
157 158 159 160 161 162 163mass0
100
%
235 236 237 238 239 240 241 242 243 244mass0
100
%
314 315 316 317 318 319 320 321 322 323 324mass0
100
%
Cl1 Cl2 Cl3 Cl4
Br1 Br2 Br3 Br4
37
4536 4538 4540 4542 4544 4546 4548 4550 4552 4554 4556 4558mass0
100
%
4524 4526 4528 4530 4532 4534 4536 4538 4540 4542 4544 4546 4548mass0
100
%
C200H320N50O50S10
FWHM=0.4 ~ 10,200 Resn
C192H290N40O40S5Cl5Br5
Isotopic Distributions at “High” m/z
4536 4538 4540 4542 4544 4546 4548 4550 4552 4554 4556 4558mass0
100
%
@FWHM=1
4524 4526 4528 4530 4532 4534 4536 4538 4540 4542 4544 4546 4548mass0
100
%
10vs16 amu
38
Mass Resolution• Mass resolution: represents the ability to separate two
adjacent masses. It measures the "sharpness" of the MS peak.
•Mass accuracy: indicates the accuracy of the mass informationprovided by the mass spectrometer
Resolution = M/ΔMNormally reported at10% or 50% valley
39mass1183 1184 1185 1186 1187 1188 1189 1190 1191 1192 1193 1194 1195 1196 1197 1198
%
0
100
%
0
100
%
0
100
%
0
100
%
0
100 1188.5654
1189.5654 1190.5654
1191.56541192.5654
1188.5654
1189.5654 1190.5654
1191.56541192.5654
1188.5654
1189.5654 1190.5654
1191.56541192.5654
1188.6514
1189.1201
Mass Resolution
FWHM = 2
FWHM = 1
FWHM = 0.5
FWHM = 0.2
FWHM = 0.1
4024.2336.965903737Cl75.77
35.4527434.968853535Cl
0.0235.967083636S4.2133.967873434S0.7532.971463333S95.02
32.06439
31.972073232S
100*18.9984018.998401919F
0.217.999161818O0.0416.999131717O99.76
15.9993315.994911616O
0.3715.000101515N99.63
14.0067614.003071414N
1.113.003351313C98.9
12.0110412.000001212C
0.012.0141022H
99.981.00798
1.0078311H
% Rel IntAv MassAcc massNominal mass
Nominal vs Monoistopic* Mass
41
Nominal vs Monoistopic vs Average MassTake for example: C19H31N4O4Cl1,nominal mass = 414
Monoisotopic mass = 414.2034
412.00 414.00 416.00 418.00 420.00 422.000.0
20.0
40.0
60.0
80.0
100.0
Average mass = 414.9267
42
Nominal vs Monoistopic vs Average Mass
284.21737284.50138284C17H32S1O1
284.27152284.47724284C18H36O2
MonoisotopicMass (C)
Average Mass(B)
Nominal Mass(A)
A: different elemental composition but same nominal mass –isobaric ionsB: calculated using C= 12.01104, H= 1.00798, O= 15.99933 and S= 32.06439C: calculated using 12C=12.0000, 1H= 1.00783, 16O=15.99491and 32S= 31.97207
43
Accurate Mass Determinations
• High resolution enables isobaric species to be differentiated based on their non-integral accurate mass.
• Consider the example below: all have a nominal mass of 28 and are therefore considered to be isobaric:CO = 27.9949
ΔM = 0.0112 M/ΔM = 2500N2 = 28.0061
ΔM = 0.0252 M/ΔM = 1110C2H4 = 28.0313These isobaric ions can be differentiated based on their accurate mass if sufficient mass resolution is employed
}}
44
Accurate Mass Determinations
• Most often employed to determine the elemental composition of an ion, usually [M]+. or [M+H]+ ion
• Experimental error minimized by co-introducing a reference compound into the source along with the unknown iePerfluorokerosene (CxFy)
• PFK used as it is mass deficient ie 12C=12.00000 and 19F= 18.99840
• Error normally expressed as ppm or millimass units (1mmu=0.001amu)
( ) 610mass true
mass observed-mass true(ppm)Accuracy Mass ×=
45
Mass Deficiency and Mass Sufficiency
• The isotopic mass is very close but not equal to the nominal mass of that isotope:
• Therefore the calculated exact mass of a molecule or of a monoisotopic ion equals it’s monoisotopic mass
• 12C is the only exception because the unified atomic mass (u) is defined as 1/12 of the mass of 12C, 1u=1.66055x10-27kg and 12C is arbitrarily assigned as 12.0000000
• As a consequence of these non-integer masses almost no combination of atoms will have the same calculated exact mass whereas they might have the same nominal mass, that is, they are isobaric
46
Mass Deficiency and Mass Sufficiency
• Mass Deficiency – the exact mass of an isotope or molecule is lower than it’s nominal mass
– eg nominal mass = 352, exact mass = 351.9897
• Mass Sufficiency – the exact mass of an isotope or molecule is higher than it’s nominal mass
– eg nominal mass = 352, exact mass = 352.0347– Only H, He, Li, Be, B and N are mass sufficient
• Atomic masses up to O are slightly higher than the nearest wholenumber while O and above are slightly less than the nearest whole number
47
Proton, Neutron and Electron Mass• Mass of proton : 1.6726 x 10-27 kg • Mass of neutron: 1.6749 x 10-27 kg
• Mass of electron: 0.00091x10-27 kg• Relative:
proton : neutron : electron1 : 1.00138 : 0.0005
Example 12C:6 protons + 6 neutrons + 6 electrons (1s2.2s2.2p2)
should = 12.01128 but in fact is 12.0107
WHY?
48
Mass Defect
• The mass of an atom is less than the total mass of the constituent protons, neutrons and electrons
• Mass defect, Δm = (Σmi) – matom and should be negative!
• This missing mass can be explained by Einstein's theory of mass-energy equivalence, E = mc2
• The deviations from whole numbers represents the energy required to bind the atomic nucleus together
• Also known as the Binding Energy, BE = Δmc2
49
• The larger the nucleus the more energy is required and the more mass deficient an isotope is:
– 4He 4.0026– 20Ne 19.99244– 40Ar 39.96238– 84Kr 83.91152– 132Xe 131.90415
• If the unified atomic mass (u) had been based on 1H = 1.00000 and not 12C/12 = 1.00000 (1H = 1.0078) then all isotopes would be mass deficient ie this is completely arbitrary and not based on some fundamental property of matter
Mass Deficiency and Mass Sufficiency
Relative to 12C = 12.00000
50
Resn~9200
PFK
PFK
PFK
308.1085 C16H20O4S11ppm error or 0.3mmu
LR EI of mw=308 (Resn~950)
Accurate Mass Determinations
51
Charge State (z>1): EI of Pyrene (70eV)
M+. 202
100
101.5
doubly charged pyrene, M++ @ m/z 101
52
EI of Pyrene at low electron energy: ~20eV
M+. 202
Note: no M++ and no fragmentation
1st IE~7.4eV2nd IE~16.6eV
53
Multiply Charged Ions: z>>1
A compound of mw A of formula CxHy
(Mass resolution is constant )
For example A=500.4
• z=1, m/z=500.4/1 = 500.4
• z=2, m/z=500.4/2 = 250.2
• z=3, m/z=500.4/3 = 166.8
• z=10, m/z= ?
Z=1
Z=2
Z=3
A
A/2
A/3
ions are 0.5 amu apart
ions are 0.333 amu apart
ions are 1amu apart
mass
%
100
mass
%
100
mass
%
100
54
Rings + Double Bonds
r+d = 1 +0.5 ΣNi(Vi-2)i
Based on valence rules the following expression can be derived:imax
Where Ni is the # of atoms and Vi is the valence of an elementUsing 0.5x(Vi-2): For monovalent elements (H, F, Cl, Br, I) = -0.5
For divalent elements (O, S, Se) = 0 and so don’t contribute to DBEFor trivalent elements (N,P) = +0.5For tetravalent elements (C, Si, Ge) = +1
r+d = 1 - 0.5Nmono + 0.5Ntri + Ntetra + 1.5Npenta + 2Nhexa + ……
Restriction to formulas of the general type, CxHyNzOn reduces theexpression to the commonly cited form:
r+d = x – 0.5y + 0.5z + 1
55
• a whole number for any OE ion• a non-integer for an EE ion
• Significance– Informs about ion type (OE or EE) and basic structural info
(number of rings + double bonds)– For EE ions, subtract 0.5 to get the right number of rings +
double bonds– Sometimes called double bond equivalents (DBE)
Rings + Double Bonds
56
Nitrogen rule
• If a compound contains an even number of nitrogen atoms (0,2,4,6…), its molecular ion will be an even mass; and if it has an odd number (1,3,5…), it will have an odd mass
• Why nitrogen?
– With the exception of N, all elements having an odd # of valences also have an odd mass (H, P, F, Cl etc)
– all elements having an even # of valences have an even mass (C, O, S, Si, etc)
– N has an odd # of valences and an even mass
• Value: places constraints on the numbers of nitrogens present
• It will be the inverse for EE ions, (M+H)+
57
• Molecular ion, M+•, most valuable information (mass, isotopic distribution, elemental composition)
• Odd electron ions, e.g. [M]+. ions, dissociate and form even electron fragment ions and neutral radicals (direct bond cleavages) or odd electron fragment ions and neutral molecules (rearrangement reactions).
• Often not stable, not detectable M+• → CI, ESI
• Requirements for an ion to be the molecular ion:•Highest mass in spectrum•Odd electron ion•High mass ions near M+• muss be explained by logical neutral losses -mass losses of 4 –14 and 21-25 highly unlikely
Interpretation of EI spectra: The molecular ion, M+.
58
• Application of the Nitrogen rule:– If a compound contains an even number of nitrogen
atoms (0, 2, 4..) its molecular ion will have an even number.
– If a compound contains an odd number of nitrogen atoms (1, 3, 5..) its molecular ion will have an odd number.
• Relative abundance of molecular ion reflects structure and stability
Interpretation of EI spectra:The molecular ion, M+.
59
Perylene – C20H12
M+.
1,3-dimethyladamantane – C12H20
M+.
Dodecane – C12H26
M+.
Ion Stability
60
Guidelines for Understanding Ion Fragmentation
• We specify the nature of the precursor ion as either– Odd electron ions (OE+.)– Even electron ions (EE+)
• Favorability of ionization sites parallels bond stability (lowest ionization energy, highest proton affinity)– Sigma < pi, < nonbonding electrons (lone pairs)
• These ions can undergo the following processes, in various combinations– Radical-site initiation– Charge-site initiation– Rearrangements – Charge retention/charge migration
61
• Fragmentation in an EI source always unimolecular (low pressure, no collision)
• Fragmentation stepwise (consecutive):[ABCD]+• → [ABC]+ + D•
[AB]+ + C•
• Fragmentation by direct bond cleavage (leads to even electron ions):[ABCD]+• → [AB]+ + CD•
example: CH3COCH3+• → CH3CO+ + CH3
•
• or fragmentation by rearrangement (leads to odd electron ions):[ABCD]+• → [AD]+• + BC
example: CH3COCH3+• → CH2=CO+. + CH4
Electron Ionization: basic mechanisms of ion fragmentation
62
Basic factors that influence the ion abundance•Stability of product ions
•Stability of the neutral (neutral loss)Neutral can be a neutral molecule or a neutral radical, where the molecule is always more stable than the radicalIn general the heat of formation of the ion is much higher than that of the neutral (i.e. the ion is more important than the neutral)
•Stevensons rule (1951):If their are two sets of ions and neutral radicals, such as
[ABCD]+• → [ABC]+ + D• or[ABCD]+• → [ABC] • + D+
than the ion of lower ionization potential will be formed preferentially
•Loss of the largest alkyl radical:If in an ion several different alkyl groups are bound to a carbon, the
largest alkyl group is lost preferentially (stability of the neutral is of importance)
63
43
73
87
101no M+.
Example: 3-methyl-3-hexanol
Basic Factors that Influence Ion Abundance:Loss of Largest Radical
C2H5 C
CH3
C4H9
OH
C2H5 C+
CH3
OH
C4H9 C+
CH3
OH
C2H5 C+
C4H9
OH
> >
m/z 73 m/z 87 m/z 101
+.
64
Radical site, charge site
• For the interpretation it is assumed in a simplistic approach that the ion has localized sites for the odd electron (radical site) and the charge (charge site - McLafferty). In reality the situation is more complex, where either the radical or the charge site may drive the reaction
Charge retention, charge migrationAssuming that upon ionization the charge remains localized at a specific site, fragmentation may either lead to charge retention or charge migration
CH3
CH3
OC
+.CH3
OC
+
+
CH3 retention
migration
65
Sigma (σ) bond cleavage• If upon ionization the electron is removed form a single (σ)
bond, cleavage of this bond is favoured. This is e.g. a typical fragmentation with ionized alkanes.
• Example – 2,2-dimethylpropaneCH3-C(CH3)3 +e- → CH3•+C (CH3)3 → +C (CH3)3 + CH3
•
H3C C(CH3)3
57
no M+.
41
57
29
66
n-decane – C10H22
3,3-dimethyloctane – C10H22
+
+
m/z113*
m/z71***
**
Sigma (σ) bond cleavage
fragments that can stabilize thecharge better are preferredie 30 > 20 > 10
67
Alpha (α) cleavage (radical site initiation)
• α- cleavage (radical site initiation) arises from the strong tendencyfor electron pairing: the odd electron is donated to form a new bond to the adjacent atom. This leads to the cleavage of the bond next to the α-atom
• The tendency to donate electrons to the adjacent bond increases in the following order: N > S, O, π, R• > Cl, Br > H.
• α- cleavage is thus particularily pronounced with amines, but also observed with ethers, ketones, olefines, alkyl substituents, while is hardly observed with halides
+.+CH3 CH2 O C2H5
+CH3 CH2 O C2H5
.
68
General Procedure for the Interpretation of a Mass Spectrum
1. Test for molecular ion identity: must be the highest peak in spectrum with even m/z value, if C, O, S, H, Cl, Br, and logical neutral losses
2. Use isotopes (13C, 34S, 37Cl, 81Br) to help deduce the elemental composition
3. If high resolution is available, deduce elemental composition
4. Ring plus double bond
5. Fragmentation pattern: important low mass series and primary neutral losses from M+.
6. Library spectra (NIST, Wiley etc)
69
Q: Assuming these ions are molecular species and were acquired under accurate mass conditions, which is the correct molecular formula?
C6F12O C22H46
C15H20N3O2Cl C23H32N5O11S2
mass308 309 310 311 312 313 314 315 316 317 318
%
0
100
%
0
100
%
0
100
%
0
100 309.1244
311.1244310.1244
312.1244
315.9757
316.9757
310.3600
311.3600
310.0843
310.5843 311.0843
70
?
1
Chemical Ionization (CI)
• Positive Ion Chemical Ionization (Munson and Field, 1966)
– Protonation by ion–molecule reaction or charge exchange (CE)
– Reactant gas at ~ 0.1-1 Torr ionized by electron ionization→ reactant ions formed by ion-molecule reactions→ low energy electron transfer reactions (CE)
– Analytes mixed in ion source with reactant gas Analyte : reactant gas = 1 : 102 – 104
– Ion source tight (higher pressure) to promote ion-molecule reactions
2
• EI produces ions which are generally high in internal energy resulting in a large degree of fragmentation and in some cases prohibits the detection of the molecular ion.
• If the pressure of a reagent gas (CH4 or NH3) in the ion source is sufficiently high (0.5 - 1 mbar) so that many collisions occur within the residence time of ions inside the source, then reactions may take place
• This is called chemical ionization, a technique whereby ions may be produced with much less internal energy (sometimes with a known amount) and less fragmentation occurs.
• The CI process most often yields even electron ions such as (M+H)+ or (M-H)- which fragment is different ways to odd electron ions.
Chemical Ionization (CI)
3
The Source
EI Source CI Source
Sample in
S
N
S
N
Trap
M+.
Filament
e-Repeller
Sample in
S
N
S
N
Trap
[M+H]+
Filament
e-Repeller
Source pressure ~ 10-6 Torr Source pressure ~ 0.1-1 Torr
4
Positive Ion Chemical Ionization
Formation of reagent ions depends on pressure and residence time:
Ammonia:NH3 + e- NH3
+. + 2e-
NH3 + NH3+. NH4
+ + NH2.
NH4+ + M MH+ + NH3
NH4+ + M [M+NH4]+
Methane:CH4 + e- CH4
+. + 2e-
CH4+. + CH4 CH5
+ + CH3.
CH3+ + CH4 C2H5
+ + H2CH5
+ + M MH+ + CH4
5
NH3CI – Formation of Reagent Ions
NH3+. NH3
+. NH4+
Low pressure – EI conditionsmid pressure – ion/moleculereactions initiated
high pressure – CI conditions
NH4+
NH3NH4+
(NH3)2NH4+
The effect of ion source pressure isclearly seen!
6
NH3CI – Formation of Reagent Ions
NH4+NH4
+
Short residence time Long residence time
NH3NH4+
(NH3)2NH4+
NH3+.
•In these experiments, NH3 pressure is constant•Residence time is changed by increasing the voltage on the repeller
7
Reagent Ion Intensity vs Source PressureIo
n In
tens
ity
ln(Source Pressure) (torr)0.1 0.5 1.0
CH4
+
5CH
+
CH4+. CH5
+
Source pressure (torr)
Inte
nsity
8
• There are 4 general pathways to form ions from a neutral analyte M in CI:
M + BH+ MH+ + B proton transferM + B [M-H]- + BH+
M + X+ MX+ electrophilic addition
M + X+ [M-A]+ + AX anion abstraction
M + X+. M+. + X charge exchangeM + X-. M-. + X
And others eg anion attachment (Cl-)
Chemical Ionization
9
• The tendency of a molecule M to accept a proton is quantitatively described by it’s proton affinity (PA):
B + H+ BH+
-ΔHr0 = PAB eg CH4, NH3
It is the negative of the enthalpy change in the gas-phase association reaction between a proton and the neutral
Thermochemical Considerations
10
Positive Ion Chemical Ionization
202NH4+Ammonia, NH3
211CH3NH3+Methylamine, CH3NH2
194C4H9+Isobutane, i-C4H10
187CH3CNH+Acetonitrile, CH3CN
182CH3OH2+Methanol, CH3OH
170H3O+Water, H2O
161C2H5+
128CH5+
Methane, CH4
101H3+Hydrogen, H2
PA (kcal/mol)Reagent IonReagent Gas
11
• In the subsequent CI experiment where:
M + BH+ MH+ + B
protonation will occur as long as the process is exothermic iePAB < PAM
This exothermicity can result in fragmentation of the MH+ ion:
Eint(M+H)+ = PAM - PAB
Thermochemical Considerations
12
Thermochemical Considerations
• Protonation under CI conditions
AB + H+ → ABH+
ΔHRx = -PA(AB)
= ΔHf(ABH+) – ΔHf(AB) – ΔHf(H+)
Rearranging yields:
ΔHf (ABH+) = ΔHf (AB) + ΔHf (H+) – PA (Proton affinity)
13
Thermochemical Considerations
• In positive chemical ionization the reactant gas and the analyte molecule compete for the proton
• Only if the proton affinity of the analyte molecule is higher than that of the reactant gas protonation can occur
• In an ideal case the difference in proton affinities is transferred as internal energy to the analyte molecule during protonation
• By proper choice of the reactant gas the ionization can be tailored in such a way that a minimum of energy is transferred to the analyte
• → can yield soft ionization with little fragmentation
14
Thermochemical Considerations
Example:
Protonation of ethylamine (PA = 208kcal/mol)• With methane (PA = 128kcal/mol)
excess energy = 208 – 128 = 80kcal/mol → strong fragmentation
• With methylamine (PA= 211)
excess energy = 211 – 208 = 3kcal/mol → little fragmentation
• If ammonia is used for CI of analytes their PA‘s determine whether a [M+H ]+ or [M+NH4 ]+ is formed:
• PA (NH3) ~ PA (analyte) → [M+NH4 ]+ and/or [M+H ]+
• PA (NH3) < PA (analyte) → [M+H ]+
• PA (NH3) > PA (analyte) → [M+NH4 ]+ or analyte not observed
15
Comparison of EI, CH4CI and NH3CIfor mw=340 species
EIno M+.
CH4CI [M+H]+
NH3CI [M+NH4]+
16
Charge Exchange Chemical Ionization
• The interaction of a positive ion with a neutral can lead to charge exchange:
X+. + M M+. + X
ΔH = IE(M) – RE(X+.) • This reaction will occur if the recombination energy (RE) of
the reactant ion (X+.) is greater than the ionization energy of the neutral M ie if the reaction is exothermic.
• Results in the formation of a radical cation (M+.) where the excess internal energy can be controlled by selection of X!
17
Charge Exchange Chemical Ionization
• Also results in some degree of selectivity as if the IE of M is higher than the RE of X, then no electron transfer will occur and M will not be observed
• Reactions of the type:
A-. + B B-. + A
ie formation of a negative ion can also occur provided the electron affinity of B is greater than the electron affinity of A.
• Rarely used in practice (+ve or –ve CECI)
18
Charge Exchange Chemical Ionization
9.3C6H6+.
9.5-10CS2+.
12.1Xe+.
13.8CO2+.
14CO+.
14Kr+.
15.3N2+.
15.8Ar+.
21.6Ne+.
Recombination Energy (eV)Ion
19
Charge Exchange Chemical Ionization
For example:
•if the IE of M is 11eV, CECI with Ne+. will yield excess internal energy of ~+10eV extensive fragmentation
•if the IE of M is 11eV, CECI with Xe+. will yield excess internal energy of ~+1eV little or no fragmentation
•if the IE of M is 11eV, CECI with C6H6+. will yield excess
internal energy of ~-1.5eV M will not be ionized
20
Negative Ion Chemical Ionization (NCI)
• Reactant Ion Negative Chemical Ionization
– Mixture of N2O and methane forms [OH]-
– M + [OH]- → [M – H]-
• that is, proton abstraction
– CH2Cl2 or CHCl3 forms Cl- by dissocaitive electron capture
• Proton abstraction [M-H]- from very acidic compounds
• Cl- attachment ion [M+Cl]- formed with acidic compounds
21
Negative Ion Chemical Ionization (NCI)
• Electron Capture Negative Chemical Ionization– 3 mechanisms of ion formation:
– M + e- M-. Resonance electron capture (0-2eV)
– M + e- [M-A]- + A. Dissociative electron capture (>2eV)
– M + e- [M-B]- + B+ + e- Ion pair formation (>10eV)
– Generation of thermalized electrons (0 to 2eV kinetic energy) bybombardment of reagent gas (methane or ....)
– Very soft ionization
– Negative ion yield increases with increasing electron affinity
– Introduction of groups with high electron affinities by derivatization such as pentafluorobenzyl derivatives
22
Summary• CI
– Analtye ions must be volatile (same as EI)• naturally, by sublimation or by derivatization (non-ionic)
– Volatility demand leads to small (<1kDa) molecules• heating biopolymers destroys them• extensive derivatization cumbersome• Desorption techniques minimize any thermal input to the analyte
(DCI)
Direct insertionheat
sample CI source CI source
sample
Desorption
1
Field Ionization (FI)• Ionization mechanism
– If atoms or molecules are exposed to very high electric fields(107 –108 V/cm) near a metal surface, a valence electron of the atom or molecule may tunnel into the anode (+vely charged)
– this is termed Field Ionization, FI (Inghram and Gomer, 1955; Beckey, 1959)
– Such high electric fields are produced if a voltage of 3 –10 kV is applied to a fine metal tip (emitter) of < 1 µm radius of curvature opposite to a counter electrode
– During ionization hardly any excess energy is tranferrred to the ion “soft ionization“ that is, little or no fragmentation
– Usually forms M+. but also [M+H]+ possible and M-.
2
Field Ionization (FI)• Ionization
– Much higher ion yields can be generated if a large number of tips are generated on a thin metal wire (3 – 10 µm i.d.) bycreation of whiskers (dendritic microneedles) by polymerizationof a suitable organic compound (benzonitrile), a processtermed activation C whiskers
– As in electron impact (EI) and chemical ionization (CI) the sample is introduced to the emitter via the gas phase
– GC, direct insertion probe, heated inlet
– Very polar, non volatile compounds can not easily be introduced
– Poor sensitivity due to low probablity of desorbed neutral coming close enough to the emitter to be ionized
3
Field Ionization: Activated Emitter
courtesy of Springer 2004
4
Field Desorption (FD)
• In field desorption mass spectrometry (FD-MS) the sample is dissolved in a suitable solvent and applied directly to the emitter. By applying high voltage to the emitter (ca. 104 V/cm) and simultaneously heating the emitter even compounds of low volatility, such as organic salts, are transferred into the gas phase
• Yields both M+. and [M+H]+ ions depending on sample polarity
• field desorption was the first mass spectrometric technique which was suited for the analysis of non-volatile compounds, such as oligopeptides, oligosaccharides and organic salts.
• Much better sensitivity than FI
courtesy of Springer 2004
5
Field Ionization and Field Desorption
courtesy of Springer 2004
6
Field Desorption – Trityl Chloride
courtesy of Springer 2004
1
Particle Bombardment
Three main techniques:
• Fast Atom Bombardment (FAB) employing 5-10keV Xeatoms
• Liquid Secondary Ion Mass Spectrometry (LSIMS) using 20-30keV Cs+ ions
• 252Cf Plasma Desorption – MeV particles created from radioactive decay of 252Cf
• allowed the MS analysis of high mass (>1000), polar, involatileand/or thermally labile species – no direct heating of sample
• rely on momentum transfer from fast moving species to sample suspended in a matrix (FAB/LSIMS) or on a foil (252Cf PD)
2
Fast Atom Bombardment (FAB)• Fast atoms are produced in a FAB gun.
• Non-volatile molecules are transferred to the gas-phase by bombardment with a beam of fast atoms (4-10 keV). (Barber et al.,1981)
Xe+. + Xeo Xeo + Xe+.
That is, a charge exchange process
8KeV 8KeV
3
FAB: Mechanism of Ion Formation
courtesy of Springer 2004
4
FAB: Mechanism of Ion Formation
courtesy of Springer 2004
5
FAB/LSIMS of Inorganic Salts
• Clusters of Cs+ with I- forms series of ions:
– +ve ion MnXn-1 eg Cs5I4+
– -ve ion MnXn+1 eg Cs4I5-
• +ve and –ve ion FAB of CsI• ions observed up to m/z >12,000• used for mass calibration in FAB
and LSIMS
courtesy of Micromass
6
FAB/LSIMS: Role of the matrix
The matrix:
• Absorbs primary energy
• Helps to overcome intermolecular forces between analyte molecules
• Helps to maintain a long lasting sample supply ie replenishes the damaged surface by diffusion
• Important for ion formation: proton donator or acceptor or electron donor/acceptor
• Sample must be soluble in the matrix
• Must be a viscous liquid that can survive the conditions in the high vacuum source to allow extended analysis
7
FAB and LSIMS: Matrices
courtesy of Springer 2004
8
FAB mass spectrum of glycerol matrix
courtesy of Springer 2004
9
1981 – the 1st analytical use of FABPeptide – 11mer
Michael Barber et al., J.C.S. CHEM. COMM., 1981
10
Cs+ LSIMS
B.N. Green et al 35th
ASMS conference - 1987
These spectra representstate-of-the-art protein analysis in 1987
Note: not m/z!
11
Surface Analysis with SIMS
• SIMS analyzes the secondary ions emitted when a surface is irradiated with an energetic primary ion beam
• Ar+, O2+, Cs+, O- are formed in a source and accelerated to
very high kinetic energies (keV) and causes the emission of secondary particles (+ve, -ve or neutral) from the surface
• This beam is rastered across the targets surface
• The secondary ions are subsequently accelerated and mass analyzed
• This technique is mostly used with solids and is especially useful to study conducting surfaces.
12
Surface Analysis with SIMS
• High resolution chemical maps ie pictures representing the chemical distribution of the surface can be produced by rastering a tightly focused ionizing beam across the surface.
• Used for trace elemental analysis especially in the semiconductor and thin coating science
• Excellent technique for the elemental analysis of solid inorganics
13
Ion Imaging
197Au and 34S signal from a pyrite (FeS2) grain
14
SIMS
Advantages:
• only surface species are ionized• depth profiling is possible by “milling” away at the sample with an ion beam• ions of all elements can be produced• can be used for small sample quantities
15
SIMSDisadvantages:
• elemental sensitivity varies (~104) between 10-4 and 10-8 mol L-1
• non-conducting samples will charge up leading to unstable signals • isobaric interferences
ie. 56Fe and 28Si2 (m/z 55.9349 and 55.9539)•this requires a resolution in excess of 5000 to distinguish by high resolution/accurate mass MS
•a double focusing sector instrument can have resolutions in the 500 to 10000 range remember, better resolution is offset by poorer sensitivity
1
Laser Desorption Ionization (LDI)
• laser pulses yielding 106 – 1010 Wcm-2 are focused on a solid sample surface of about 10-3 – 10-4 cm2. • The laser pulse ablates material from the surface, creating a microplasma of ions and neutral molecules.
eg. CsI(s) Cs(CsI)n+
• LD is used to study surfaces since you can good spatial resolution with such a small beam of photons• high sensitivity• large variation in ionization probability ie. different energy to vaporize and ionize different samples
hυ
2
LDI
• large spread in ion kinetic and internal energies, normally only fragments of the sample are seen in the mass spectrum due to dumping so much energy into the molecules, therefore structure is destroyed• useful for metals, inorganic salts and some polymers• signals are very short, therefore LD is best used with a mass analyzer such as TOF
3
Matrix Assisted Laser Desorption Ionization (MALDI)
• the compound to be analyzed is mixed in a solvent containing an organiccompound (the matrix) which strongly absorbs at the laser wavelength.• the solvent is evaporated off leaving the analyte embedded in the matrix material.• an intense laser pulse deposits large amounts of energy into the sample in ashort period of time.• this ejects or ablates bulk portions of the solid which contain matrix and analyte molecules from the surface
4
MALDI
• both UV and IR lasers can be used but most often a N2 (UV@337nm) laser is used• little internal energy is transferred to the analyte due to expansion andevaporation of the matrix material from the analyte so there is little fragmentation• ionization reactions can occur at any point in the process but the origin of ionsproduced in MALDI is not fully understood with numerous possibilities:
•desorption of preformed (M+H)+ and (M+Na)+ ions•gas-phase protonation•direct photoionization M+. and M-.
5
MALDI
• among the chemical and physical ionization pathways suggested for MALDI are: gas-phase photoionization, excited-state proton transfer, ion/molecule reactions, or desorption of preformed ions.
• the most widely accepted mechanism involves gas-phase proton transfer in the expanding plume with photoionized or photoexcitedmatrix molecules.
• since most matrix materials contain aromatic rings, they can actas energy gathering chromophores.
M + hυ M*M* + A AH+ + (M-H)-
M* + M MH+ + (M-H)-
MH* + A AH+ + M
M = Matrix A = Analyte
6
Laser Desorption and Ionization: Mechanism
courtesy of Micromass (Waters)
7
Laser Ionization (without matrix): ion emission as a function of λ
courtesy of Micromass (Waters)
Absorption spectrum of matrix Absorption spectrum of sample
8
Laser Ionization (with matrix – MALDI): ion emission as a function of λ
courtesy of Micromass (Waters)
9
MALDI: Matrices
courtesy of Springer 2004
10
MALDI Target - Batch Introduction Process
courtesy of Springer 2004
Bruker Micromass
Can be fully automated!
11
MALDI
courtesy of Springer 2004
MALDI spectrum of an N-linked glycan
12
MALDI–Tof of a monoclonal antibody (m/z ~ 150,000)
13
Protein Identification using MALDI
• Large proteins (>100,000 Da) may be multiply charged (doubly or triply charged): [M+H]+, [M+2H]2+, [M+3H]3+ but no more - very unlike ESI!
• Smaller proteins and peptides are always singly charged – again, this is not the case for ESI
• MALDI typically exhibits better sensitivity than ESI because it has a higher tolerance for other non-peptide sample constituents -attamole
• MS/MS of [M+H]+ ions provides fewer structurally significant fragment ions than does [M+2H]2+ ions commonly seen in ESI
• not as useful for peptide sequencing or MS/MS ion database searching
• Difficult to interface to chromatography• Also used for synthetic polymer characterization and imaging
14
2D Gel Electrophoresis
15
Protein Identification using MALDI
• Separate proteins on a 2D polyacrylamide gel (2D-PAGE)
• Excise individual spots
• These spots, which may contain 1 or more proteins, are degraded into small peptides (enzymatically) and measured by MALDI (or ESI)
• The resulting MALDI mass spectrum (primarily [M+H]+ ions) is converted into a table of molecular weights of the individual peptides present to yield a Peptide Mass Fingerprint
• Peptide Mass Fingerprint (PMF) or peptide mapping is an ideal method to identify peptides derived from a protein which are already known and in a database
• The quasimolecular ions of this mixture of smaller peptides provide a map or fingerprint which can be searched against protein databases to provide a protein identification
16
Peptide Mass Fingerprint using MALDI
1500 2000 2500 3000 3500 m /z
0
5000
10000
15000
a.i.
17
MALDI-Tof of Polystyrene
Reproduced from Schriemer & Li, 1996
(A) mwt~330,000
(B) mwt~600,000
(C) mwt~900,000
18
MALDI Imaging
Courtesy of S. Khatib-Shahidi, M. Andersson, J. L. Herman, T. A. Gillespie, and R. M. Caprioli. Anal. Chem. 2006, 78, 6448-6456.
1
• Inductively coupled plasma used originally and still used today in emission spectroscopy
• Plasma temperature may exceed 8000oC
• Elements with IP < 10 eV fully ionized → mass spectrometry• Inorganic samples first digested (e.g with nitric acid), pneumatically
nebulized and introduced as finely dispersed mist into an argon ICP at +1200 Watt
• Coupled to quadrupole MS and to magnetic sector double focussing instruments (the latter have much better mass resolution)
• Very sensitive, very specific
• Can suffer from isobaric interferences
Inductively Coupled Plasma (ICP) MS
2
ICP-MS
3
ICP-MS
• The Ar plasma is generated and maintained at the end of the glass torch located inside the loops of a water cooled copper load coil.
• A radio frequency (RF) potential applied to the coil produces anelectromagnetic field in the part of the torch located within its loops.
• A short electric discharge from a wire inside the torch providesthe electrons to ignite the plasma.
• In the electromagnetic field of the load coil these electrons are accelerated and collide with Ar flowing through the torch producing Ar+. ions and free electrons.
4
ICP-MS
• Further collisions cause an increasing number of Ar atoms to be ionized and result in the formation of plasma.
• The plasma-forming process rapidly becomes self-sustaining and may be maintained as long as Ar gas continues to flow through the torch
• These colliding species cause heating of the plasma to ~10,000 K. The high temperatures rapidly desolvate, vaporize, atomize and ionize the sample. Therefore the sample is turned into atomic ions which are then mass analyzed
5
• Each element shows up at its own m/z value, including isotopes
• Intensities are directly proportional to the amount of element introduced to the torch
• No structural information since complete atomization occurs
• Different ionization efficiencies result in different sensitivity
• Isobaric interferences:
• ArO+ m/z 55.9573 / Fe+ m/z 55.9349
• Ar2O+ m/z 95.9197 / Mo+ m/z 95.9068
• Ar2O++ m/z 47.9599 / Ti+ m/z 47.9479
ICP-MS
6
ICP-GCMS – Organotin standards
110.00 115.00 120.00 125.000.0
20.0
40.0
60.0
80.0
100.0
Sn isotopic distribution
120Sn+ monitoredDetection Limit:1. inorganic Sn – not reported2. MBT 4.4fg3. TPrT 5.3fg4. DBT 9.4fg5. MPhT 4.4fg6. TBT 9.9fg7. DPhT 10fg8. TPhT 11fg
1μL injection of 5ppb standard
0 15105 Retention time (min)
2,000
10,000
8,000
12,000
4,000
6,000
ICP
-MS
Inte
nsity
1
Atmospheric Pressure Ionization (API)• conventional ionization methods employ sources that are at high
vacuum (EI, CI, FI/FD, FAB/LSIMS, MALDI) and/or temperature (EI, CI, FI/FD)
• the introduction of API sources employing a number of different types of ionization has allowed very robust instruments to be developed for LC/MS
• These “new” ionization techniques have greatly extended the range of analytes that can be studied by MS to compounds that are high molecular weight, thermally labile and polar.
• While the sources are designed to operate at atmospheric pressure we must still maintain a high vacuum in the rest of the instrument if we want to perform mass spectrometry!!
2
Capillary
HPLC inlet
Nebulizer
Waste
heated N2
Nebulizergas inlet
Skimmers
Octopole
++
+
++
++ ++ + + ++ + + +++
LensesVacuum Wall
API Source
Vacuum Pumps
Mass analyzer
}
Atmospheric pressure }
reduced pressureHigh vacuum
Spray is at right anglesto entrance to
MS - orthogonal
courtesy of Agilent
3
• High vacuum must be maintained in the mass analyzer and detectorregion even though the source is at atmospheric pressure
• The region after the source is heavily pumped with rotary vacuum and turbomolecular pumps (usually)
• Also, a series of skimmers and flow restrictors are placed between the source and the mass analyzer region
• These skimmers allow ions to be efficiently transmitted to the high vacuum region while at the same time allow air, solvent vapours and other neutral volatile species to be pumped away
• The exact design will depend on the specific instrument type andmanufacturer
API Source
4
• Electrospray (ESI)• high flow rate (100μL/min – 1mL/min)
• capillary flow rate (2μL/min - 100μL/min)
• low flow rate (<2μL/min)– nanospray (200-500nL/min) – ESI is most sensitive at these
low flow rates
• Atmospheric Pressure Chemical Ionization (APCI)
• Atmospheric Pressure PhotoIonization (APPI)
• Atmospheric Pressure MALDI
API Sources
}pneumaticallyassisted ESI
5
Relative Applicability of API Techniques
ESI: Electrospray Ionization & APMALDIAPCI: Atmospheric Pressure Chemical IonizationAPPI: Atmospheric Pressure Photo Ionization
EI, CI, GC-MS
Mol
ecul
ar W
eigh
t
Analyte Polarity
ESI & APMALDI
1000
100,000
10,000
nonpolar very polar
APCI & APPI
6
Electrospray (ESI)• Based upon the electrostatic spraying of liquids where a solution is
passed through a needle held at high voltage (kV) relative to a counter electrode (the entrance to the MS)
• When the solution contains an electrolyte and the needle forms part of the API source then the fine mist of droplets that emerge from the needle tip possesses a net +ve or –ve charge determined by the polarity of the needle and the solution chemistry of the bulk liquid
• These preformed and then sprayed ions, which are characteristic of the dissolved analytes, are attracted to the entrance of the MS by applying appropriate voltages
7
Electrospray (ESI)
• The formation of the spray must be aided by nebulization (pneumatically assisted) at liquid flow rates higher than a few μL/min
• ions exist in solution, if not, electrospray doesn’t work, it is not an ion formation technique rather than a technique for extracting ions from the solution-phase into the gas-phase free of solvent for mass spectral analysis
• The analyte must be an ion in solution either as a preformed ion such as or through modifying the solution chemistry to induce a charge
• This can be accomplished by changing solution pH or adding cations egLi+, NH4
+ etc or anions to form adducts eg Cl-, OAc- etc
N
8
Electrospray Ionization
+ ++
++
++
++
+-
--
-
-
CoulombicExplosions
+
+++++--
+
+++++ --
RayleighLimit
Reached
+ ++
++
++
++
+-----
Evaporation
+
+ Analyte Ion(proton transfer andadduct ions)
Solvent Ion Cluster
Charged Dropletscontaining ions in solution
Analyte Ions in the gas phase- both +ve and -ve
Nebulizer assisted >1μL/min- capillary 2-100μL/min- normal 0.1-1mL/min
“Classical” - nanospray < 1μL/min
9
The “Source”
Taylor cone
++++
++++++++
++ +
+++++++
+ ++++++ + +++++++
+
+
High voltagePower supply -
electrons
Anode -oxidation
+
+
+
+
+
+
-+ +
+ +
++
+
+
+
---
-
-
- +++
++
++
++
+
+++
+
+++
+
+++
+
++
++
++
++
+ +
cathode - reduction
to MS
10
Proposed Mechanisms:1. Charge Residue Model: where the droplet is completely evaporated
leaving “bare’ analyte ions
2. Ion Evaporation Model: field assisted ion desorption
• Requires ~ 107Vcm-1 and a final droplet diameter of 10nm
• Fits well with the observed data
• In either case it is required that the analyte be an ion in solution (+veor –ve) or made to be charged by modifying the solution to cause the analyte to be ionized
• This can be accomplished by changing pH, adding modifiers (Na+, Li+)
11
Electrospray Solution Chemistry• Mobile phase pH has a major effect for analytes that are ions in solution:
– Basic pH for negative ions
– Acidic pH for positive ions
• Changing pH can enhance performance for analytes that are not normally ionized in solution
Positive Ion ModeR1 R1| |
:N - R2 + HA +HN - R2 + A-
| |R3 R3
Base Acid Analyte Ion
O O|| ||
R-C-OH + :B R-C-O- + H:B+
Acid Base Analyte Ion
Positive ion mode, [M+H]+
Negative ion mode, [M-H]-
12
• In the case of acid/base chemistry, ideally we want to be 2 pH units either side of pK in order to cause complete protonation (+ESI) or deprotonation (-ESI) to give maximum sensitivity
• In the case of batch introduction (infusion) of sample this is easily accomplished however in the case when LC is employed it is the nature of the mobile phase that determines the ions we will observe and the sensitivity
• For example, in a reversed phase (C18) separation of analytes, in order to achieve a good separation it is necessary for the analytes to be neutral in solution so that they may interact with the stationary phase and achieve a good separation. These neutral species will not yield the best sensitivity when ESI is used.
Electrospray Solution Chemistry
13
• Don’t forget, the ESI process is a competition for charge!
• A neutral in solution will pick up charge in a variety of ways and while we can influence which process is favoured we can not eliminate all competing ion formation mechanisms
• Not only do proton transfer reactions occur but adduct ion formation is commonly observed
• Species such as [M+NH4]+, [M+Na]+ and [M+K]+ in positive ion and [M+OAc]- and [M+Cl]- in negative ion are often observed even though these modifiers may not have been deliberately added to the solution containing the analyte
Electrospray Solution Chemistry
14
+ESI of Nucleotide Homologue (mw=890)Sample in 1:1 CH3CN/H2O+0.2% formic acid
[M+H]+
[M+NH4]+
[M+K]+
[M+Na]+
15
Electrospray Considerations
Samples:
• Ions in solution: catecholamines, sulfate conjugates, quaternary amines, carboxylates, phosphorylated compounds
• Compounds that can have a charge induced: carbohydrates• Compounds containing heteroatoms: carbamates, benzodiazepines• Multiply charged in solution: proteins, peptides, oligonucleotides• A curious feature of ESI is the formation of multiply charged ions ie
where z>>1 and sometimes as high as 100
16
Electrospray ConsiderationsSolution Chemistry Parameters:• flow rate• sample pK, solution pH• solution conductivity
Samples to Avoid:• extremely non-polar samples: PAHs, PCBs• Samples containing high levels of buffers/electrolytes as this will
cause ion suppression
Ion Suppression:
• Competition and interference with analyte ionization by other endogenous matrix species resulting in decreased number of ions characteristic of the analyte(s)
17
Protein ESI-MS
• In this mass spectrum, each peak represents the quasi molecular ion of the protein with one more charge attached, usually, but not always, a proton (H+) eg m/z 942.6 is the [M+18H]18+
• Consequently, each peak can be used to calculate the mwt of the protein and the resulting values averaged across all charge states.
• This results in mass accuracies for protein mwt determination of + 0.01% or better depending on the type of mass spectrometer employed.
18
• Let the unknown mass of the protein be M and the # on charges be ncorresponding to the addition of (M+nH)+
• For 2 adjacent measured masses m1 (high mass) and m2 (low mass) we can write 2 equations:
m1 = (M+n) (i) and m2 = (M+n+1) (ii)n (n+1)
Solving for n:for the ion at m/z 998.0 (m1) = (M+n) 998n = M+n
nfor the ion at m/z 942.6 (m2) = (M+n+1) 942.6n+941.6 = M+n
(n+1)
Consequently: 998n = 942.6n+941.6 n =17 for m1 (m/z 998)
Substituting n=17 in (i) gives M = (m1n)-n = (998x17)-17 = 16,949
• These laborious calculations can be performed for all ion in the distribution or a software deconvolution can be performed
Protein ESI-MS
19
+ESI of a ~39kDa Protein - Infusion@1μL/min
m/z1150 1160 1170 1180 1190 1200 1210 1220 1230 1240 1250
%
0
100
[M+33H]33+ [M+32H]32+
[M+18H]18+
[M+22H]22+
[M+50H]50+
m/z200 400 600 800 1000 1200 1400 1600 1800 2000 2200 2400 2600 2800
%
0
100
20
Software Deconvolution
Software manipulation of the full scan +ESI data to show protein mwt
mass39300 39400 39500 39600 39700 39800 39900 40000 40100
%
0
10039,643+1.3
21
pH=2.6
pH=3.0
pH=5.2
• the charge states of the gaseous ions generally represent the charge states in the condensed phase. These are sometimes modified by ion/molecule collisions. Ions such as large biomolecules are highly charged.
• the transfer of ions to the gas phase is not an energetic process. Ions are cold, in fact the desolvation process further cools ions.
• non-covalent interactions can be preserved when the species enters the gas phase. This is significant for the application of ESI to the study of biological molecules such as proteins.
ESI mass spectra of bovinecytochrome c
22
Raffinose – trisaccharide, mwt=504 +ESI
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500 525 550 575 600
%
0
100
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500 525 550 575 600
%
0
100
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500 525 550 575 600
%
0
100
in 1:1 MeCN/H2O+5mMNH4OAcm/z 522 (M+NH4)+
In 1:1 MeCN/H2O+0.2%FA m/z 505 (M+H)+
m/z 522 (M+NH4)+
+LiOAc
m/z 511 (M+Li)+
23
Raffinose – mwt=504 +ESI vs -ESI
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500 525 550 575 600
%
0
100 m/z 503 (M-H)-
m/z 549 (M+HCOO)-
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500 525 550 575 600
%
0
100
In 1:1 MeCN/H2O+0.2%FAm/z 505 (M+H)+
m/z 522 (M+NH4)+
24
Not Always Protonated! decamethylferrocene
m/z100 120 140 160 180 200 220 240 260 280 300 320 340 360 380 400 420 440
%
0
100
m/z80 100 120 140 160 180 200 220 240 260 280 300 320 340 360 380 400 420 440
%
0
100
M+.
M+.
M+.+ESI in 1:1 MeCN/H2O+0.2%FA
+ESI in MeCN
EI
ie no (M+H)+ observed!Electron transfer dominates
Oxidation
Fe
25
• Electrospray ionization (ESI) has allowed mass spectrometry to investigate a huge diversity of molecules that were very difficult or impossible to study by MS previously
•proteins, DNA, RNA, oligonucleotides•polymers, non-volatile inorganic and organometallic molecules and salts
• As a result it has completely revolutionized mass spectrometry.
• It has also revolutionized the sales of mass spectrometers as the can be considered to be an analytical technique for biochemistry (big $$).
• Also, it has spurred the growth of more sensitive and exotic types of MS and combinations of MS analyzers.
ESI – a MS Revolution
26
Atmospheric Pressure Chemical Ionization (APCI)
• gas phase chemical ionization (CI) process where the vapourized LC mobile phase acts as the CI reagent gas to ionize the sample
• Mobile phase and analyte are first nebulized (N2) and vapourised by heating to 350-550oC
• The resulting vapour is ionized using a corona discharge (source of electrons)
• Subsequent ion/molecule reactions (CI) then cause ionization of the analyte
• Unlike ESI, analyte ions do not need to exist in solution
• Unlike ESI, best sensitivity is achieved at high liquid flow rates ie 200μL –1mL/min therefore easily interfaced to conventional HPLC
• Analytes must be thermally stable and “volatile”
27
APCI
28
Analyte containing aerosol
APCI Process
Charged reagent gas formed
+
++
+
+
+ +++
+ +
+
++
++
++
+
+++
+
Vapour
Heat and N2 to aid volatalization
+
Analyte ions
Charge transfer to analyte eg H+ transfer, charge exchange etc
+ ++
+
kV corona discharge- a robust source of e-
needle
29
APCI Considerations
Samples:
• Compounds of intermediate mwt and polarity: PAHs, PCBs, fatty acids, steroids, phthalates.
• Compounds that don’t contain acidic or basic sites (e.g. hydrocarbons, steroids, alcohols, aldehydes, ketones, and esters)
• samples containing heteroatoms: ureas, benzodiazepines, carbamates
• samples that exhibit a poor electrospray response, that is, APCI can be considered to be complimentary to ESI
30
APCI Considerations
Solution Chemistry Parameters:
• less sensitive to solution chemistry effects than ESI – ion suppression not so important
• Best sensitivity at higher flow rates than ESI
• accommodates some non-polar solvents not compatible with ESI (hexane, CH2Cl2 etc)
Samples to Avoid:
• thermally labile, polar and high mwt compounds due to the vaporization process
31
APCI Mechanism
S + e- → S+. + 2e-
• Solvent molecules are ionized (S+.)
• the solvent is usually a complex mixture of H2O, CH3CN/CH3OH and mobile phase modifiers
S+. + S → [S+H]+ + S[-H]• S+. abstracts a hydrogen atom ie a CI process
[S+H]+ + M → [M+H]+ + S• [S+H]+ ionizes analyte M by proton transfer or proton abstraction
S+. + M → M+. + S• charge transfer can also occur with solvents like CH2Cl2
32
Atmospheric Pressure Photo-Ionization (APPI)
• Experimentally, you can view APPI as an APCI source where the corona discharge has been replaced with a Kr lamp
• The 1st step is complete vapourization of the mobile phase used in the LC separation employing nebulization (N2) and heating to 350-550oC
• gas phase photoionization process• where the vapourized mobile phase may be photoionized to
form a CI plasma• or a modifier (dopant) is added to aid the photoionization
process and formation of the CI plasma• or the analyte can be directly photoionized by photons from
the Kr lamp
33
Atmospheric Pressure Photo-Ionization (APPI)
• It is ionized by high energy photons from a Kr lamp (usually) causing either direct or indirect (dopant) photoionization
• Very useful for non-polar analytes that are difficult to ionize with ESI or APCI such as PAH’s
• Unlike ESI, best sensitivity is achieved at liquid flow rates around 200mL/min therefore easily interfaced to conventional HPLC
34
APPI Process
Vapour
Dopant is photoionized and acts as reagent gas –Indirect
Evaporation
Analyte containing aerosol
Analyte ions+
+
++
+
+ +++
+ +
+
++
++
+
++
++
+
+
Photon ionizes analyte - Direct
+
+ ++
+
+
++
+
+
hυ
hυ
Dopantadded
35
APPI Mechanisms
Direct APPI:
M + hν → M+. + e-
Analyte molecule M is ionized to molecular ion M+.
– If analyte ionization potential is below Kr lamp photon energy
Subsequently:
M+. + SH → [M+H]+ + S•
Molecular ion M+. may abstract a hydrogen to form [M+H]+
ie a CI process
36
APPI Mechanisms
Dopant APPI:
D + hν → D+. + e-
• Photoionizable dopant D is in excess & yields many D+. ions
D+. + M →→ [M+H]+ + D• Analyte M ionized by proton transfer from dopant or solvent
D+. + M → M+. + D• D+. ionizes analyte M by electron transfer ie charge transfer
37
Energetics for PhotoionizationPhotoMate™ lampKrypton 10.0 eV, 10.6 eV
Ionization Potentials (IP)Anthracene 7.4 eVFluoranthene 7.8 eVCaffeine 8.0 eV4-Nitrotoluene 9.5 eV2,4,6-Trinitrotoluene 10.59 eV
Dopant Ionization PotentialsToluene 8.82 eVAcetone 9.70 eV
Solvent Ionization PotentialsMethanol 10.85 eVAcetonitrile 12.19 eVWater 12.61 eV
• The photons from the Kr lamp can only photoionize compounds of lower IP
• Common HPLC solvents like H2O, CH3OH and CH3CN are NOT ionized and therefore cannot aid ion formation
• In this circumstance, only direct photoionization of the analyte can yield characteristic ions such as M+. (not very efficient)
– Subsequent ion/molecule reactions can form [M+H]+
• Dopants are used that will be ionized by the Kr lamp
38
Electrospray (ESI)• Volatility not required
• Preferred technique for polar, high mwt, thermally labile analytes
• Ions formed in solution
• Can form multiply charged ions
APCI/APPI• Some volatility required
• Analyte must be thermally stable
• Ions formed in gas phase
• Forms singly charged ions only
Atmospheric Pressure Ionization Techniques
39
Ionization of Analytes
How do we choose which technique to use?– is the analyte volatile?
– is the analyte thermally labile?
– Does the analyte have heteroatoms that can accept (N > O) or lose (O >> N) a proton?
– accepts a proton - use positive ion mode
– loses a proton - use negative ion mode
Ion Suppression?– Dirty matrix would favour the use of APCI/APPI rather than ESI
because they are more tolerant to matrix effects than ESI
40
Chromatographic ConsiderationsESI:
• Concentration dependant
– smaller i.d. column gives better sensitivity - nanospray at 200-500nL/min
• However also works well from 1µl/min to 1 ml/min
• Post-column addition can be used to adjust ionization chemistry
APCI/APPI:
• Mass flow dependant
– column i.d. has little effect on sensitivity
• Works well from 100 µl/min to 1.5 ml/min
• Can be used with normal phase chromatography
41
General Mobile Phase Considerations
• Metal ion buffers interfere with ionization
• Surfactants/detergents interfere with evaporation
• Ion pairing reagents can ionize and create a high background
• Strong ion pairing with an analyte can prevent the analyte from ionizing
• Some mobile phase additives will cause persistent background problems
– TEA interferes in positive ion mode (m/z 102)
– TFA interferes in negative ion mode (m/z 113)
42
ESI:• Solution pH must be adjusted to create analyte ions
– pH 2 units away from pK of analyte
• Organic modifier (CH3OH/CH3CN) has little effect on ionization
• Volatile buffer concentration should be <25mM
• Non-volatile buffers should be avoided or their concentration should be very low <<5mM
• Na+ and K+ adducts commonly occur
Mobile Phase Considerations
43
APCI/APPI:• Organic solvent should be a good charge transfer reagent
– use methanol instead of acetonitrile
– proton affinity of CH3OH (182kcal/mol) vs CH3CN (187kcal/mol)
• Chlorinated solvents can aid ionization in negative mode
• Volatile buffer concentration should be <100 mM
• Non-volatile buffer concentration should avoided or be very low <<5mM
• Ammonium adducts may occur with ammonium salt buffers
• APPI may require a dopant (eg acetone)
Mobile Phase Considerations
44
Mass Spectra of Prednisolone in Negative Mode APCI
[M+Cl]-with CH2Cl2
Prednisolone does not normally ionize in negative mode APCI. In the presence of CH2Cl2, a very intense [M+Cl]- ion is formed.
m/z150 200 250 300 350 400
0
100000
200000
300000
400000
500000
600000
Abundance 395.
337
7.3
365.
3
335.
3
421.
3
no CH2Cl2
m/z150 200 250 300 350 4000
100000
200000
300000
400000
500000
600000
Abundance
O
O
O H
O H
HO
45
Mass Spectra of Curcumin in Negative Mode APCI
m/z100 200 3000
10000
20000
30000
40000
50000
60000
70000
80000
90000367.0
337.0
307.1217.1160.9m/z100 200 300
0
10000
20000
30000
40000
50000
60000
70000
80000
90000367.1
337.1
307.1191.1
with CHCl3 no CHCl3[M-H]- [M-H]-
Curcumin is an example of a phenolic compound that ionizes equally well in the presence of oxygen or CHCl3.
O
HO
O
O
OOH
46
Caffeine
ESI APCI APPI
m/z200 400 600 8000
20000
40000
60000
80000
100000
120000
140000 Max: 13143
195.
1 217.
1
[M+H]+= 195
m/z200 400 6000
20000
40000
60000
80000
100000
120000
140000 Max: 71549
103.
212
1.2
195.
119
6.1
[M+H]+= 195
m/z200 300 400 500 6000
20000
40000
60000
80000
100000
120000
140000 Max: 148840195.
119
6.1
[M+H]+= 195
courtesy of Agilent
47
Methomyl
ESI APCI APPI
m/z200 400 600 8000
10000
20000
30000
40000
50000
60000
70000
80000
90000Max: 206617
163.
116
5.1
185.
018
6.1
347.
134
8.1
[M+H]+= 163
m/z200 400 600 8000
10000
20000
30000
40000
50000
60000
70000
80000
90000Max: 95891
106.
116
3.1
164.
1
[M+H]+= 163
m/z200 400 600 8000
10000
20000
30000
40000
50000
60000
70000
80000
90000Max: 3663
163.
1[M+H]+= 163
courtesy of Agilent
48
Budesonide
ESI APCI APPI
m/z200 400 600 8000
20000
40000
60000
80000
100000
120000
140000 Max: 161681
413.
243
1.3
453.
2
[M+H]+= 431
m/z200 400 600 8000
20000
40000
60000
80000
100000
120000
140000 Max: 78432
103.
212
1.2
323.
234
1.2
395.
241
3.2
431.
3
[M+H]+= 431
m/z200 400 600 8000
20000
40000
60000
80000
100000
120000
140000 Max: 140093
413.
243
1.2
[M+H]+= 431
courtesy of Agilent
49
Sample Matrix Effects
The MS hardware is robust and tolerates non-volatile components
however…
The ionization process is effected by the concentration and type of salt/buffer and results in “Ion Suppression” and is much more prevalent in ESI
“Competition and interference with analyte ionization by other endogenous matrix species resulting in decreased number of ions characteristic of the analyte(s)”
50
mAU
10
20
sulfa in water
sulfa in water
sulfa in water
sulfa in HBSS
sulfa in HBSS
sulfa in HBSS
50000100000150000
2000
4000
min1 2 3 40
UV
EIC, m/z 285
TICScan mode
Signal suppression!
Sample Matrix Effect in ESIComposition of HBSS:
Component g/L
Sodium chloride 8Calcium chloride 0.1Potassium chloride 0.4Potassium phosphate monobasic 0.06Magnesium sulfate 0.1Sodium bicarbonate 0.35Sodium phosphate dibasic 0.048Glucose 1Phenol red 0.011
Sulfachloropyridazine (mwt=284) dissolved in water vs. Hanks Balanced Salt Solution (HBSS)
courtesy of Agilent
51
• Replace non-volatile buffers with volatile buffers at a concentration of <10 mM for ES or <100 mM for APCI.
• Substitute phosphates, sulfates, and borates with ammonium acetate or formate, trifluoroacetic acid (TFA), heptafluorobutyric acid (HFBA), tetrabutylammonium hydroxide (TBAH)
• If a non-volatile buffer must be used, use a buffer where only the anionic or cationic part is non-volatile, i.e. ammonium phosphate, not sodium phosphate.
• Keep the pH the same using volatile additives:Formic acid, acetic acid, TFA, ammonium hydroxide
• Volatile ion pair reagents should be employed such as HFBA
Adapting Existing LC Methods to LC/API-MS
52
Summary of Ionization MethodsCompound volatile or semivolatile:
• Electron impact (EI):• M+• and perhaps substantial fragmentation
• Chemical ionization (CI):• Positive chemical ionization, [M+H]+ (soft ionization - little fragmentation)
• Negative chemical ionization (electron capture), [M]-. (soft ionization - little fragmentation, can be very sensitive)
• Field Ionization (FI):• M+•, (soft ionization - little fragmentation)
Compounds non-volatile, methods difficult to couple to HPLC:• Field Desorption (FD):
• [M+H]+, [M+Na]+ (soft ionization - little fragmentation)
• Fast Atom Bombardment (FAB) and Liquid Secondary Ion Mass Spectrometry (LSIMS):
• [M+H]+ , [M+Na]+, [M-H]- (soft ionization - quasimolecular ion and fragment ions)
53
Summary of Ionization Methods
Compounds non-volatile, methods difficult to couple to HPLC:• MALDI: [M+H]+, [M+Na]+, [M-H]- some multiple charging observed (both soft
and hard ionization, quasi molecular ion and fragment ions, biopolymer analysis)
Compounds non-volatile, methods can readily be coupled to HPLC• APCI: [M+H]+, [M+Na]+, [M+NH4]+, [M-H]- (soft ionization, low to medium
molecular weight, medium to high polarity)
• APPI: M+•, [M+H]+, [M-H]- (soft ionization, low to medium molecular weight, medium to high polarity)
• ESI: [M+H]+, [M+nH]n+, [M+Na]+, [M+NH4]+, [M-H]-, [M-nH]n- (soft ionization, low to high molecular weight, medium to high polarity, biopolymers and organic salts)
1
Mass Separation
• Magnetic sector instruments– Single focussing with magnetic sector (B)
– Double focussing with a combination of magnetic and electric sectors (EB or BE)
• Linear quadrupoles (Q - mass filters)
• Three dimensional quadrupoles (ion traps - IT)
• Linear ion traps (2D)
• Time of flight mass spectrometers (Tof)
• Fourier transform ion cyclotron resonance (FTICR or FT-MS)
2
Mass Separation and the Lorentz ForceNOTE:
• All mass analyzers function on the basis of the Lorentz Force equation which describes the force exerted on a charged particle in an electromagnetic field. The particle will experience a force due to the electric field (qE), and due to the magnetic field (qvB). Combined they give the Lorentz force equation:
F = qE+qvB
– F is the force (in newtons) – q is the electric charge of the particle (in coulombs) = ze– E is the electric field (in volts per meter) – B is the magnetic field (in webers per square meter, or equivalently,
teslas) – v is the instantaneous velocity of the particle (in m/s)
q = ze therefore, F = zeE+zevB
3
Mass Separation: Magnetic Fields (B)Deflection of ions in magnetic fields:
an ion of mass m and charge z moving with velocity, v, that traverses a magnetic B at right angles to the direction of the field will follow a circular path of radius r that fulfills the condition of equilibrium of FL (Lorentz Force) and centripetal force FC (from the source accelerating voltage)
FL = qvB = mv2/r = FC r = mv/qB
Right hand rule for a +ve charged particle moving through a magnetic field:
Fingers in the direction of BThumb in the direction of vPalm in the direction of the experienced force
4
This shows the working principle of a magnetic sector - the radius, r through which the ion will be deflected depends on themomentum (mv) of the ion ie the magnetic sector is a momentum analyzer not a direct mass analyzer!
Since the initial kinetic energy of the ions is given by:zeV = mv2/2 where V is the accelerating potential
And rearranging for v2: v2 = (2zeV)/m (i)
From: zevB = mv2/r we can derive v2 = (zeBr)2/m2 (ii)
Substitute v2 from (i) in (ii) and rearrange: m/z = eB2r2/2V
Mass Separation: Magnetic Fields
5
m/z = eB2r2/2V
• Therefore specific values of V and B allow ions unique in m/z to pass to the detector. Variations in V or B will cause ions to collide with the walls of the flight tube therefore at any unique value of V or B only one specific ion will be passed to the detector. In practice only B scans are preferrred when generating full scan data over a large (>50Da) mass range
• One exception to this is when high resolution, accurate mass measurements are made where Vacc scanning is preferred as voltages can be controlled and measured much more accuartely than can B
Mass Separation: Magnetic Fields
6
Resn~9200
PFK
PFK
PFK
308.1085 C16H20O4S11ppm error or 0.3mmu
LR EI of mw=308 (Resn~950)
Accurate Mass Determinations
7
Deflection of ions of different masses in a constant magnetic field
•This is how Aston’s original mass spectrograph operated!• In modern instruments, the magnetic field is scanned to bring ionsof different m/z ratios successively to the detector
8
Directional (angular) focusing of a magnetic field
Divergent ions of the same m/z will be brought into focus by a magnetic field
9
Mass Separation: Magnetic Fields
• One significant drawback with employing B scans is that the initially accelerated ions have a kinetic energy spread which exhibits itself as increased peak width ie low resolution.• To overcome this problem an electric sector (ESA) is combined with the magnetic sector to produce what is called a double focusing instrument.
10
Principle of the Electrostatic Sector (ESA)• Remember the Lorentz Force equation which describes the
force exerted on a charged particle in an electric fieldF = qE
• If a radial electrostatic field E is created between 2 curved plates held at oppositely charged potentials of +E and –E, an ion of charge z moving with velocity v will traverse this field when its electrostatic force equals the centripetal force:
zeE = (mv2)/rAnd since the kinetic energy of an ion 1/2mv2 = zeV, then
r = 2V/E
Note: the trajectory is independent of m and z and so the ESA is not a mass analyzer but reduces kinetic energy dispersion which results in narrower peaks and increased mass resolution
11
Double Focusing Mass Spectrometers
• Many geometries have been tried however in general they can be categorized as:– Normal or Forward geometry where:
Source ESA Magnet Detector
• and:– Reversed geometry where:
Source ESAMagnet Detector
12
Double Focusing (Nier Johnson):Reverse Geometry
13
Double Focusing (Mattauch-Herzog geometry)
Double focusing in a plane → photo plate
14
Mass Resolution: Definition
10% Valley
δm10%
δmFWHM
m
10% Valley
δm10%
δmFWHM
m
• The 10% valley definition: δm = the mass difference between two peaks which are separated by a valley equal in height to 10% of the height of the smallest peak
• The full width at half maximum (FWHM) definition: δm = the width of a peak at half-height
15
Mass Resolution
• The FWHM definition is easier to apply (only need one peak), but gives a resolution about twice that of the 10% valley definition
• Resolution for sector instruments is usually given as the 10% valley figure.
• High resolution has some obvious advantages:
-It allows one to resolve ions that are isobaric-The narrower a peak, the easier it is to measure its
position accurately
16
Mass Resolution
• Low resolution: <2,000. Suitable only for nominal mass measurement.
• Medium resolution: 2,000-20,000. Suitable for accurate mass measurement. Resolve isotope clusters of high charge states.
• High resolution: >20,000. Better than medium resolution. You can never have too much resolution!
• In practice, there is a trade-off between resolution and sensitivity. The ions are not coming from a point source: they exit the source through a slit of finite dimensions, and cannot be perfectly focussed. Slits and lens help to compensate for this by cuttingout ions from the centre of the beam and focussing. To get veryhigh resolution, the slits have to be narrowed, which means thata lot of ions are lost.
17
How Many Possible Elemental Compositions?
1961832345104517123447900
11113202005999731964800
9710101083215381046700
364550155257505600
33322164115266500
13217233778400
611271124300
1111223200
1111112150
5ppm3ppm0.1ppm1ppm3ppm5ppm10ppmMol mass
5% isotopic accuracy
2% isotopic accuracy
without isotope abundance information
18
• No difference between high mass accuracy in the low m/z range and 3ppm mass accuracy and 2% isotopic abundance accuracy
• Magnetic sector – 1 to 5ppm• FTICRMS – 0.5 to 1ppm• Tof – 1-10ppm• Orbitrap – 1-5ppm
How Many Possible Elemental Compositions?
19
“New” Developments in Magnetic Sector Instruments
• Large, high field magnets
– Mass range up to 10,000 Da at full accelerating potential (10 kV) for analysis of large biopolymers
– Example: bovine insulin (MW 5734)
• Laminated magnets– To reduce magnetic hysteresis– Total cycle time < 1 sec, fast scanning
20
Linear Quadrupoles (2D - mass filters)
21
Linear Quadrupoles (2D - mass filters)
• Four hyperbolic rods (cheap version: circular rods) – compromise!• Opposite pairs of rods are connected electrically but are of
opposite polarity• Each pair of rods has a DC (U) + AC (V0 cosωt) Rf voltage applied:
1 pair of rods: -(U + V0 cosωt) and the opposite pair: +(U + V0 cosωt) where, ω = radial frequency = 2πf
• During a mass scan, the DC and AC voltages are ramped but the ratio of DC/AC (ie U/V0)is kept constant
• For a given DC and AC amplitude, only ions with a given m/z (or m/z range) have stable oscillations and are transmitted and can be detected
22
Quadrupole (end view)
Hyperbolic Round
Equipotential Field Lines
23
Superposition of RF and DC Voltages Applied to Rods
4000
3000
2000
1000
-1000
-2000
-3000
-4000
500
-500
0VOLTAGE
(V)
ATOMIC MASS UNITS
(u)
RF VOLTAGE
6000 V P/P
AT 2500 u
dc VOLTAGE
500 V AT 2500 u
24
Ion Motion
+ve ion
DC +
+
X
Z
DC -
-
Y
Z
+ve ion
AC +
+
X
Z
+ve ion
AC-
-
Y
Z
+ve ion
+ve ion
AC+DC-
-
Y
Z
•This motion is very complex!•DC fields focus +ve ions in the +ve plane anddefocus them in the –ve plane•The superimposed AC helps correct this defocusingeffect
25
Linear Q: Equations of MotionFrom the electrical part of the Lorentz equation, we can derive the equation of motion (x and y directions) for a particle in a combination of DC and AC Rf fields the Mathieu equation:
– u represents the x or y transverse displacement. We do not consider displacement in the z direction because the electric field is 0 along the asymptotes of the hyperbolic rods.– The 2 parameters characteristc of the field (a and q) are given by:
d ud
a q uu u
2
2 2 2 0ξ
ξ+ − =( cos )
220
8ϖmr
zeUaa yx =−= 220
4ϖmrzeVqq yx
−=−=
and
26
• Where the variable ξ is the time in radians of the applied field = ωt/2
• U is the DC voltage and V is the AC Rf voltage of frequency ω• r0 is the radius of the instrument aperture
• Plotting a against q gives the Mathieu stability diagram of the linear quadrupole field - a/q = 2U/V
• Typical values are:
- U = DC voltage (~200 - 1000V)
- V = AC voltage (~1000 - 6000V, 1-2MHz),
- m = mass of ion, e = electonic charge, z = # of charges on ion
- 2r0 = distance between the rods - 1-2 cm
Linear Q: Equations of Motion
27
Stability Diagram
28
aq Space
• Note:
– Both +ve and –ve abscissa with a values ranging up to 10 and q values ranging up to 20
– In practice we only operate in the +ve area of region I
Why?
– Because in order to have a and q values >1 we would require VERY high DC and AC voltages which is not practical
29
Stability Diagram
X unstable
L1, only 1 ion has a stable trajectory allothers ions are lost therefore adjacentions are resolved from each other
L2, 3 ions have a stable trajectoryat the same time therefore these3 ions would not be resolved fromeach other
In practice, the ratio of a/q is changedby changing the DC voltage
0.1
0.80.4
0.3
0.2
a
q
Y unstable
X and Y Stable
L1
L2
L1 = L2
Operating linesa/q constant . .
.... ..
..
What would happen if noDC voltage is applied?
30
Ion Motion
31
Conceptualizing a Q scan
0.1
0.80.4
0.3
0.2
a
q
m1 < m2 < m3
stable region of m1
stable region of m2
stable region of m3
Operating or scan line
32
Mass Range and Resolution• Depends on 5 parameters:
• Rod length (L) – 50 to 250mm• Rod diameter (r) – 6 to 15mm aligned to μm accuracy• Maximum supply voltage (Vm)• AC (Rf) fequency (f)• Ion injection energy (Vz) - ~5 volts
• From the theory of quadrupole operation the following relationship can be derived:
Mmax = 7x106Vm/f2r2
Consequently, as r and f increase, Mmax decreases and as r and f decrease, Mmax increases
33
• The resolution limit of a quadrupole is governed by the number of cycles of the Rf field to which the ions are exposed:
M/ΔM = 0.05 fL m/2eVz
Mass Range and Resolution
2
• Consequently, as both f and L increase so does resolution. If L in increased then f can be decreased and vice versa
• Scanning speeds as high as 6,000 amu/sec and mass resolution of 10,000 is attainable
34
Linear QAdvantages:
• Small and light weight ~1 foot long
• Inexpensive
• Simple to operate – complete computer control
• Low accelerating voltage – handles high source pressures better
• Full scan mass spectra and selected ion monitoring (SIM) for quantitation
Disadvantages:
• Unit mass resolution only and limited mass range
• High mass discrimination
• Rod contamination causes further imperfections in the quadrupole field – compromises resolution and sensitivity
35
Linear Q
Other applications:
• QQQ for MS/MS
• Hybrid instruments eg BEQQ and QqTof
• Ion lenses (hexapoles and octapoles)
• Collision chambers for MS/MS ie QQQ and BEQQ etc
• Prefilter – before mass resolving rods to reduce contamination
36
Quadrupole 3D Ion Trap (QIT)
Ion trap consists of three electrodes:
• ring electrode (hyperbolic shape)
• 2 hyperbolic electrodes - end caps
• Orifice for ion injection
• Orifice for ion ejection
• Pulsed introduction of ions
Cap
Cap
Ring
Cap
Cap
Ring
Cap
Cap
Ring
Cap
Cap
Ringr0
37
• Ions accumulated in the trap ie “trapped” and then further experiments can be performed on the trapped population of ions eg MS or MS/MS or even MSn
• During this time, ions are gated away from the IT and lost• employs:
- AC (Rf) to trap and scan ions out to detector – no DC component- He buffer gas necessary for efficient trapping of ions directed into the ion trap
He present at all times therefore no delay between MS and MS/MS experiments
Quadrupole 3D Ion Trap (QIT)
38
QIT (properties)
• Ion trap volume very small (7mm i.d.)• High sensitivity (10-18 mol) (scan mode)• High mass range : 6,000• Higher mass resolution than Q ~x2-3• High dynamic range: 106 depending on space charging• MSn capabilities• Low mass cut-off is a disadvantage• Helium is introduced intentionally into the ion trap (10–3 mbar)
– Needed as a buffer to absorb kinetic energy of incoming ions without chemical interaction so they can feel the effect of the trapping field - dampening (cooling) of oscillations
– collision partner for MS/MS and MSn
• Ions are concentrated in center of ion trap• Better resolution and better sensitivity than Q
39
QIT (ion motion)
• Between the three electrode a quadrupole field exists, which forces the ions to the center of the trap
• The farther the ion is removed from center of trap the stronger is the exerted electric force
• The ions oscillate within the trap, but with a rather complex sinusoidal motion
• The ion motion can be described by Mathieu’s differential equations
40
Quadrupole 3D Ion Trap (QIT)• For the QIT, the electric field has to be considered in 3 dimensions. The electric field can be descibed by the expression:
Φx,y,z = Φ0(r2 - 2z2)r0
2
• The equations of ion motion in such a field are:
d²z/dt² - (4e/mr0²) [(U - V cos2ωt)z = 0d²r/dt² + (2e/mr0²) [(U - V cos2ωt)r = 0
• Solving these Mathieu type differential equations yields the parameters az and qz
az = -2ar = 16eU/(mr0²ω²) and qz = -2qr = 8eV/(mr0²ω²)Where ω = 2πf, f = fundamental Rf frequency of the trap (~1MHz)
41
QIT (Ion stability diagram)
courtesy of Spektrum Akademischer Verlag
Ring Electrode
Ring Electrode
Endcap
Endcap
q = 0.908
q < 0.908
42
QIT (stability diagram)
• Ions are only stable both in r and z direction for certain defined values of a and q
• Ions oscillate with so called “secular frequency”, f, which differs from the frequency of applied Rf field because of inertia (in addition oscillations of higher order)
• Ions of different m/z are simultaneously trapped, V determines low mass cut-off at qz = 0.908, which increases with V
43
QIT (mass selective ion stability scan)
• Mass scan is possible by increasing the amplitude of the voltage on the ring electrode (U = 0, az = 0 ie no DC voltage)
• Scan line: While scanning along this line (a=0) ions become increasingly non stable and exit the stability diagram at qz = 0.908.
• Trajectory of these ions in z- direction.
• Ions exit from trap through holes in end cap.
• Linear scan function
44
• An additional Rf voltage with low amplitude is applied to end caps.
• If frequency of this additional voltage is equal to frequency ofoscillating ions, ions take up energy exponentially and become non stable:
→ Resonance ejection ( at q < 0.908)
• Mass scan with resonance ejection leads to– Higher resolution– Higher sensitivity– Higher mass range– Faster scanning – up to 26,000 amu/sec– Improved reproducibility due to higher net ion sampling
rate
QIT (resonance ejection)
45
QIT: Mass Scan – resonance ejection
• 1: Clear Trap
• 2: Accumulation Time
• 3: Scan Delay
• 4: Mass AnalysisCourtesy of Agilent
46
Space Charging
530m/z
0
20
40
60
80
100
Rel
ativ
e A
bund
ance
524.3
525.3
526.3
5300
20
40
60
80
100524.4
525.4
526.3527.5
5300
20
40
60
80
100524.5
525.5
526.5
527.5
5300
20
40
60
80
100 524.8
525.7
526.7
522 522 522 522
~ 300 Ions ~ 1500 Ions ~ 3000 Ions ~ 6000 Ions
Good resolutionand mass accuracy
Poor resolutionand mass accuracy
Courtesy of Agilent
47
QIT (space charge)
• With increasing number of ions trapped the space charge increases
• Space charge distorts the electric field
• Deterioration of resolution, sensitivity and mass accuracy
Solution:
Pre-scan or measure in real time to control the number of ions (or more correctly, the number of charges)
in the trap (a maximum of ~103 - 104)
48
Linear (2D) traps
• Similar idea to 3D traps with a “new” 2D geometry
• Rf only quads with DC voltage end electrodes
• Larger size than 3D IT – higher ion capacity (~x50) therefore fewer space charge problems
• More than one design for this type of trapping instrument
• Hybrids such as QQQ where Q3 can also be used as a linear trap and LT-FTICR
49
AxialTrapping
Exit Lens
Radial Trapping RF Voltage
Radial Trapping RF Voltage
AxialTrapping
DCVoltage
Resonance Excitation
Trapping Forces in a Linear Ion Trap
Courtesy of Sciex
50
Linear Ion Trap – 2nd design
DC 1 DC 2
z
y
• For Axial Trapping 3-130 V DC3>DC2>DC1
• To Contain ions: DC1=DC3>DC2
Radial Quadrupolar Trapping1.2 MHz 5KV0-P
DC 3
DC 1 DC 2 DC 3
RF - RF -
RF +
RF +
x
y
Radial Dipolar Excitation5-600 KHz 0-400 Vpp
AC+ AC -
GND
GND
x
y
Courtesy of Thermo
51
Linear Ion Trap vs 3D Trap
No low mass cut-off
Trapping Efficiency: >10
Detection Efficiency: doubled
Overall Efficiency: >10
Ion Capacity (Spectral): >20
Scan Rate (amu/sec): 4x
Highly Efficient MSn: 5x over 3D IT
52
Time of Flight (Tof)Principle:
Ions of different mass (accelerated by the same field, V) have different velocities and thus flight times. The larger the mass the slower the ion:
zeV = mv²/2
Ion formation:
Ions are introduced to the Tof in pulses (e.g. MALDI or orthogonal extraction from a continuous beam such as ESI)
Ion detected by analogue or time to digital converter (GHz ADC or TDC)
• Linear Tof (high mass range but low mass resolution)
• Reflectron Tof (lower mass range but high mass resolution)
53
Mass Separation: Time of Flight (Tof) MS
acceleration region(drift region)
54
Basic PrinciplesSince the initial kinetic energy of the ions is given by:
zeV = mv²/2 (i)velocity: v = (2zeV/m)1/2 (ii)time of flight: t = L/v = L[m/(2zeV)]1/2 (iii)
m/z = 2eVt2/L2 (iv)Example:
For C6H5+. and C7H7
+., (m/z 77 and 91), accelerated at 10kV, what are the velocities of these 2 ions and how long would it take them to traverse a 2m flight tube?using eqn (ii) v77 = (2x1x1.6022x10-19x10,000/m)1/2
m(kg) = 0.077/6.022x1023 = 1.279x10-25
v77 = 128,759m/s 15.53μssimilarly for v91 v91 = 118,457m/s 16.88μs
V is the extraction pulse potential (V)L is the length of field free drift zone (m)t is the measured time-of-flight of the ion (s)e = 1.6022x10-19C
55
Example cont• From eq (iii), difference in flight time:
tA/tB = (mA/mB)1/2
• Consequently, this square root relationship causes Δt for a given Δm/z to decrease with increasing m/z
• For example:Δt/amu is calculated to be 114ns at m/z 20
to be 36ns at m/z 200to be 11ns at m/z 2000
• Tof mass analyzer depends on the ability to accurately measure these short time intervals to make it a useful MS
56
Linear Tof• Transmittance as high as 90%• Ions introduced into the flight tube have a temporal and kinetic
energy distribution which yields relatively poor mass resolution. • Kinetic energy spread can be reduced by employing Delayed Ion
Extraction
Principle of Delayed Ion Extraction:
• Ions are formed during a short pulse of a few nanoseconds• The acceleration (extraction) field is only applied after a delay of
some hundreds of nanoseconds:• At the beginning of the extraction ions with high initial velocities
have traveled further than slower ones. Therefore after the second extraction pulse they do not experience the full acceleration potential.
• Thus the initially faster ions will be accelerated less than the initially slower ions.
57
Reflectron TofSame m/z butdifferent kineticenergy
• In a reflectron Tof, the ions traverse the drift tube and penetrate into an electric field (ion mirror) where their direction is reversed.
• Faster ions (with higher kinetic energy) penetrate farther into the electric field than slower ions (with lower kinetic energy).
• Thus faster ions have a longer flight path and therefore need approximately the same flight time as the slower ions which have a shorter flight path.
58
Tof: Advantages and Disadvantages• Extreme mass accuracy
– reflectron ~ 5-10ppm
– limited with quadrupole MS, poor with ion traps and linear Tof
• High mass resolution
– reflectron ~5,000 to 20,000
– Quadrupole MS, ion traps and linear Tof operate closer to unit mass resolution at m/z ~ 103
• Extreme mass range
– linear >105 Da, reflectron <104 Da
– Ion traps and quadrupoles are limited to ~6,000 Da
• Acceptable linearity for linear and reflectron Tof
– not as good as quadrupole MS, but similar to ion traps
• Very good scan-to-scan reproducibility for linear and reflectron Tof
– as good as quadrupole MS
59
Fourier Transform Ion Cyclotron Resonance (FTICRMS – FTMS)
Principle:
An ion of velocity v entering a uniform magnetic field B perpendicular to its direction will move on a circular path by action of the Lorentz force, the radius rm is given by:
rm = mv/qB
Upon substitution with v = rmω, the cyclotron angular frequency ωc
becomes:
ωc = qB/m• cyclotron angular frequency is independent of ions initial velocity but is a function of it’s mass, charge and the applied magnetic field
• once trapped, the ions oscillate with a cyclotron frequency that is inversely related to their m/z ratio
60
FTICR MS• Basic Construction:
– a cell where ions are trapped by intense, constant magnetic field and applied voltage
– The cell accepts ions in a “pulsed” mode from the continuous ion beam– Detection of the ions is based on the FT deconvolution of the image
current the circulating ions induce in a pair of detector plates after excitation with a resonant Rf pulse.
61
FTICR MS cont.
• MS/MS:Excitation of the ion is achieved using a variety of techniques. Namely:
– Sustained off-resonance Irradiation Collision-Induced Dissociation (SORI-CID)
– Infrared Multiphoton Dissociation (IRMPD)
– Electron Capture Dissociation (ECD)
– Blackbody infrared radiative dissociation (BIRD)
• High sensitivity and >105 mass resolution
• MS/MSn
• Cyclotron frequencies can be measured with very high accuracy and precision leading to ultra high resolving power and high accuracy mass measurements
62
Ion Trapping and FTICR MS
• ions enter the cell (or are created internally) and they begin their cyclotron motion, orbiting around the centre of the magnetic field
• since the magnetic field is quite high (typical minimum of 4.7T, but this is increasing) the ions are trapped in the radial (x,y) direction.
• Resolving power and scan speed increase linearly with B
63
• by applying small, equal potentials to the two end or “trapping”electrodes, the ions are confined in the z or axial direction.
• ions can be confined for very long periods of time such that ion/molecule reactions or even slow unimolecular dissociation processes can be observed and monitored.
Ion Trapping and FTICR MS
64
FTICR MS Detection• In FT detection, all ions, regardless of their mass are detected at the
same time.
• Once ions are trapped inside the ICR cell they are excited by a fast sweep of all the Rf frequencies, exciting the ions to cyclotron motion with a larger radius.
Ions before excitation.They have their naturalcyclotron radius within the magnetic field.
65
FTICR MS - Detection
• All ions are resonantly excited for the same amount of time.• Each ion retains its characteristic cyclotron frequency (depending on
m/z) but their radii of orbit increase.• After excitation all ions have the same radii of motion since they were
irradiated with Rf of the same amplitude for the same amount of time.• Once the Rf is turned off, each ion packet, consisting of ions of the
same m/z value induces an image current on two sets of receiver plates which are part of the ion cell.
Before excitationAfter excitation
66
FTICR MS - Detection
When a packet of ions (+ve) approaches an electrode, electrons are attracted from ground and accumulate in that electrode causing a temporary current.
As the ions continue to orbit, the electrons accumulate in the other electrode. The flow of electrons in the external circuit represents an image current. The amplitude of the current is proportional to the number of ions in the packet.
67
FTICR - Detection
• the frequency of the image current oscillation is the same as the frequency of the ion’s cyclotron motion which is related to mass. A small AC voltage is created across a resistor and is amplified and detected.
• using FT techniques all ion packets, each containing ions of the same mass, are detected. The decay of the image current (as the excited cyclotron orbit radius decays) is detected in time and transformed into a frequency domain signal by a Fourier transform.
Rf Excitation
Detected time domainimage current
Resulting mass domainSpectrum
Fourier Transform
Time
Time
m/z
68
FTICRMS• Very high resolution is possible. The current record is 8x108,
and routine values are 100,000 or so.• Long trapping times are possible, allowing for ion-molecule
reactions.• Good sensitivity.• Like the ion trap, the FTICR cell works well with pulsed
sources.• MSn capability• However, expensive because of the cost of superconducting
magnets and the very high vacuum requirements.• Difficult to operate
69
FTICRMSSample: very complex crude extract
from human blood plateletsAmount: unknown, but very low conc.Flow: 200 nl/minScan Cycle: 1 spectrum every 3.5 s
HCT116_A_030523101055 # 2189 RT: 72.26 AV:1 NL: 7.84E4T: FTMS + p ESI Full ms [ 200.00-2000.00]
300 400 500 600 700 800 900 1000 1100 1200m/z
0
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
Rel
ativ
e Ab
unda
nce
579.29291
857.44525
557.31122
279.15924891.38403
654.25793301.14130
400.23349 1157.58093
RT:
40 45 50 55 60 65 70 75 80 85 90 95 100 105 110Time (min)
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
Rel
ativ
e Ab
unda
nce
78.81
86.60
49.33
72.26
66.96
100.26
Expand
HCT116_A_030523101055 # 2189 RT: 72.26 AV:1 NL: 7.84E4T: FTMS + p ESI Full ms [ 200.00-2000.00]
550 555 560 565 570 575 580 585 590 595 600 605m/z
0
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
Rel
ativ
e Ab
unda
nce
579.29291R=315540
557.31122R=323474
574.33777R=312472 595.26740
R=300047
RP: 400,000 @ m/z 400
Courtesy of Thermo
70
FTICRMS Resolution
Courtesy of IonSpec
1
Hyphenation in Mass Spectrometry
• Gas Chromatography – Mass Spectrometry (GC-MS)• Liquid Chromatography – Mass Spectrometry (LC-MS)• MS-MS and MSn - Tandem Mass Spectrometry
WHY?• the ability to interface an orthogonal separation technique to
MS greatly increases the information content that can be derived from complex mixtures
2
Gas Chromatography – Mass Spectrometry (GC-MS)
• Both are gas phase techniques although at somewhat different pressures:
• Ion source normally at high vacuum (EI and CI)• GC operates at ~ 5-10psi
Quite a stable and “friendly” relationship – they just get alongas both are gas-phase processes
GC MS
3
GC-MS
• Coupling of capillary GC to MS simple, as low carrier gas flow rates (1-2 mL/min) easily tolerated by MS vacuum system.
• Carrier gas always helium (low viscosity, low mass).
• Fused silica capillary introduced directly into the ion source via a transfer line which must be heated.
• Operation modes of a GC/MS:– Full scan → TIC/RIC– Selected Ion Monitoring (SIM)
4
Operating Modes• Full scan
– selective, sequential transmission of ions to the detector in a continuous fashion (BE, EB, Q, QQQ, 3DQIT)
– qualitative information
• Selected Ion Monitoring (SIM or SIR)– Mass analyzer jumps from one pre-selected m/z value to the next
– Only the response from the selected ions is recorded – no mass spectra
– Detector time for the selected ions is increased by a factor of 10 – 100 and so is the sensitivity
– Used for quantitative analyses – target compound analysis
• Example:– If a Q is scanning from m/z 100 – 1100 in 1sec then each ion is recorded for
1msec
– If the same Q is set to jump between only 4 ions in a SIM experiment then each ion is recorded for 250msec
5
GC-MS: Full Scan
6
GC-MS: Selected Ion Monitoring (SIM)
7
Liquid Chromatography – Mass Spectrometry (LC-MS)
Historical approaches:
• There is a basic compatability problem when an LC is interfaced to a MS:
– LC: 25-50oC, 200nL/mim – 1mL/min liquid flow rate at 100-3000psi
– GC: 50-300oC, 1mL/min He(gas) at 5-10psi
– MS: 200oC, 1x10-6mbar (high vacuum) and 20mL/min gas flow
• The vacuum problem – gas load:
• 1mL/min of hexane(l) yields approx 172mL/min gas
• 1mL/min of water(l) yields approx 1240mL/min gas
• Conventional MS can pump ~20mL/min of gas and maintain high vacuum
• Atmospheric Pressure Ionization solves many of these problems
8
Liquid Chromatography – Mass Spectrometry (LC-MS)
• In GC, the “mobile phase“ normally referred to as the carrier gas is He and is easily removed however in LC the mobile phase is a complex mixture of solvents which might contain buffers, pH modifiers and/or ion-pair reagents – much more difficult to volatalize and remove
• LC is most commonly used for compounds that are not easily analyzed by GC because they are thermally unstable, involatile or high mwt
• MS requires species in the gas phase therefore we must transfer these difficult compounds into the gas phase without chemical or thermal modification
9
LC-MS: a difficult courtship
Clearly defined boundary(picture courtesy of P.J. Arpino)
• It is the function of the interface to “blur” the distinction between the gas and liquid phase as far as the MS is concerned
• Q: does the fish fly or does the bird swim?• A: a good question – compromise! Perhaps the bird doesn’t
realize it is swimming and the fish doesn’t realize it’s flying!
MS
LC
10
LC-MSWhy LC-MS?• LC is capable of providing separation of compounds unsuitable for
GC (even with derivatization)• Polar, ionic, involatile, high mwt and thermally labile analytes are
readily chromatographed by LC• Sample clean-up can be more straight forward for LC• LC allows selection of stationary and mobile phase• Conventional detectors (UV, FL etc) exhibit good detection limits
but have limited specificity• The MS is a universal (sometimes), sensitive and highly specific
detectorHOWEVER:
• A GC column is much more efficient than an LC column ieHETP
11
Solutions to the Problem:• There are 2 basic approaches to the problem of interfacing an LC to a
MS:
– The “spray” type interfaces which introduce all or a portion (splitting) of the LC eluent to the source :
– Direct Liquid Introduction (DLI)
– Thermospray (TSP)
– Continuous Flow FAB (CF-FAB)
– Atmospheric Pressure Ionization (ESI, APCI and APPI)
– The “enrichment” type interfaces which preferentially remove the LC solvent from the less volatile analytes before introduction to the source:
– Moving Belt
– Particle Beam
• This is by no means an complete list but describes the most important
12
Direct Liquid Introduction (DLI)
• Liquid is introduced directly into the high vacuum source– 10 – 40μL/min of liquid– Sprayed through a 2-5μm laser drilled hole – prone to blockage– Desolvation chamber vapourizes analyte and liquid– Vapour enters CI ion source– Proton transfer and proton abstraction dominates– Only CI type spectra with mobile phase forming the CI plasma– Only volatile buffers can be used– Works well for reversed and normal phase solvent systems
13
Thermospray (TSP)
• Capillary is heated to partially vapourize the mobile phase supersonic jet of vapour and liquid
• Mobile phase @ 1mL/min must contain a volatile buffer - normally NH4OAc• Reversed phase only ie solubilize the NH4OAc• Ionization occurs through ion/molecule reactions with either NH4
+ or OAc-
• Resulting mass spectra are NH3CI like in +ve mode• Much more robust than DLI but classical TSP limited to reversed phase separations• This can be overcome to some extent by employing an alternative form of ionization
such as a discharge voltage (APCI like) then termed Plasmaspray or a heated filament as in a conventional EI/CI source (fragile)
14
Continuous Flow FAB
15
• Analyte introduced continuously to the probe tip at 5 –10μL/min and normally contains a small amount of a matrix eg glycerol
• Tip is irradiated with a beam of Xe0 or Cs+ which causes sputtering of ions into the gas phase
• Good for polar, thermally labile species but sensitivity can be 3-6 orders of magnitude lower than ESI
Continuous Flow FAB
16
Electrospray (ESI)
•Electrospray (nanoESI)•up to 1 µl/min •Concentration dependant•Most sensitive
•Pneumatically assisted electrospray• flow rate range 5µl/min –1mL/min• sensitivity poorer than nanoESI• Concentration dependant• More robust
17
ESI
• All API sources/interfaces work because while the source is at atmospheric pressure the MS analyzer is at high vacuum.
• A series of skimmers and vacuum pumps is placed between the source and the MS to reduce pressure from AP to HV
• Orthogonal spraying helps reduce the gas load into the MS
In-line spraying - most modernsources are orthogonal ie at rightangles to the entrance to the MS
18
ESI – Remember!
• Droplets are highly charged during the spraying process and Coulombic repulsion causes the spray to “explode” into smaller drops as the solvent evaporates
• As the droplets become smaller the charged analyte ions will be desorbed into the gas phase (IEM) or as the droplet becomes completely dry (CRM) and then extracted into the MS
• Orthogonal source designs now ie sprayer at right angles to the entrance to the MS
19
APCI
20
APCI• Advantages:
– Entire mobile phase and sample vaporized into the gas phase (with heat), then ionized
– Accommodates high LC flow from (0.2 - 2 mL/min)
• Uses heat (400–500 °C) and nebulizer gas to vaporize HPLC eluent and transfer sample into the gas phase for APCI
– Temperature setting is not critical
– Sensitive
• Disadvantages:
– Thermally labile analytes may degrade when vaporized
– Low molecular weights only
– CI mass spectra only, little fragmentation typically
21
APPI
courtesy of Applied Biosystems
22
APPIAdvantages:
– Entire mobile phase and sample vaporized into the gas phase (with heat), then ionized
• Uses dopant (Toluene/Acetone) to promote ionization– Accommodates high LC flow from (0.2 - 2 mL/min)
• Uses heat (400–500 °C) & nebulizer gas to vaporize HPLC eluent and transfer sample into the gas phase for photoionization
– Detection limits are very good• Improvements over ESI and APCI compound dependant
– Wider application range (low to medium polarity compounds)Disadvantages:
– Thermally labile analytes may degrade when vaporized– Low molecular weight compounds only (<1000)
23
Moving Belt
• LC eluent is mechanically transported from the column (A) to the high vacuum ion source (B)
• Combination of differentially pumped regions (1,2,3) and heating (4) removes solvent
• The dried sample is flash vapourized into the source (EI/CI) or irradiated with Xe0 or Cs+ ions (FAB/LSIMS)
A
B
3 4
2 1
24
Moving Belt
• The polyimide belt contributes to the chemical noise of the system
• Mobile phases containing high H2O concentrations are difficult to handle
• Latent heat of vapourization of H2O is very high (compared to organic solvents)
• Can bead on the belt (high surface tension) – destroys chromatographic integrity
• Mechanically very complex - poor reliability• One of the first LC/MS interfaces available (along with DLI)
25
Particle Beam
26
Particle Beam
• LC eluent introduced with He to generate an aerosol of solvent droplets• Solvent evaporates and the resultant beam of dry particles, He and
solvent vapour enters a momentum separator which preferentially removes low mwt species (He and solvent)
• Dry particles enter a conventional high vacuum EI/CI source• 0.1 – 1mL/min flow rates accommodated• Samples must be volatile and thermally labile and mwt<1000
27
Tandem Mass Spectrometry – MS/MS• The combination of 2 or more stages of mass analysis in one experiment
• These stages are decoupled from one another in one of 2 ways:
– MS/MS in space, where parent ion selection, dissociation and subsequent mass analysis are physically performed in different regions of the MS eg BE/EB, QQQ, Tof-Tof etc
– Hybrid instruments, where 2 different types of mass analyzer are put together eg QTof, QTrap etc
– MS/MS in time, where parent ion selection, dissociation and subsequent mass analysis are performed in the same region of the MS but are decoupled in time ie they are performed as a series of timed events following one another eg 2D and 3D ion traps, FTICRMS
• The dissociation step is typically achieved using Collision Induced Dissociation (CID) sometimes called Collisional Activation (CA)
28
Ion Stability
• 3 “types” of ions based on the mass spectrometric time frame:
– Unstable – dissociate quickly ie before leaving the source k > 106s-1 and are never observed
– Metastable – dissociate after leaving the source but before detection 105s-1 < k < 106s-1 can be detected
– Stable – arrive intact at the detector k < 105s-1
• In order to perform MS/MS we must somehow destabilize the “stable” ions and cause them to dissociate
• There are a number of ways to accomplish this but the most common is Collision Induced Dissociation (CID)
29
Collision Induced Dissociation (CID)
• An ion/neutral species interaction wherein the projectile ion isdissociated as a result of interaction with a target neutral species (N2, Ar, He). This is brought about by conversion of part of the translation energy of the ion into internal energy of the ion during collision.
AB+ + Ncg AB+* A+ + B + Ncg
• The internal energy (IE) of AB+* is composed of IE prior to collision (usually low) and the amount Q, transferred during collision:
EAB+* = EAB+ + Q
vibrationally andelectronically excited
30
CID• The absolute upper limit for Q is defined by the “centre of mass” collision
energy, ECM)ECM = ELAB mN
mN+mAB
Where: ELAB user set collision energymN is the mass of the target or collision gasmAB is the mass of the ion
• ELAB can be in the 1-10keV range for BE/EB and Tof-Tof instruments – single or double collisions, He employed with short collision cells
• ELAB can be in the 1-200eV range for QQQ, QIT, Q-Tof instruments employing multiple collision events with Ar, N2 or He (for QIT) and longer collision cells
• Scattering can be an issue• Very fast process – 10-15 s• Must not ionize the collision gas in the collision event
( )__________
31
CID• For example:
– an ion of m/z100 with a collision energy of 50eV colliding with He will gain a maximum of 50*(4/(100+4)) = 1.9eV.
– consequently, in the 1-200eV collision regime, we usually employ N2 or Ar as the collision gas to maximize the energy transfer
– the same ion with 5 keV, colliding with He could in principle pick up 190eV of internal energy, and no doubt some do, but very, very few are seen.
– consequently, in the keV collision regime, we usually employ He as the collision gas to minimize ion scattering and prevent excessive fragmentation
32
CID• In high energy CID in a sector instrument, we expect to see only the products of
glancing collisions which do not knock the ions out of the beam, and because such experiments are carried out under single-collision conditions (each precursor ion undergoes a maximum of one collision), the total internal energy is relatively low, say 1 – 15 eV.
• As a general rule, the bigger it is, the harder it is to break. A simple way of understanding this is to keep in mind that the energy deposited in the ion may not be localized, and in any case, rapidly distributes over the bonds of the ion. Bigger ions more bonds less energy/bond, and less chance that a given bond will have enough energy to break.
• A CID type process can also occur in the source of an API instrument because ions are accelerated (focused) through a high pressure region before they enter the mass analyzer – this can cause “unstable” ions to collide with neutral gas molecules and dissociate in the source – called “in-source CID”
33
“In-source” Collision Induced Dissociation (CID)mwt=451
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500
%
0
100 452.175
396.128453.198
m/z100 125 150 175 200 225 250 275 300 325 350 375 400 425 450 475 500
%
0
100 396.128
352.143
164.071452.198
397.145 474.184
“normal” cone voltage165V
“low” cone voltage65V
[M+H]+
[M+H]+
Ions moving quickly throughhigh pressure region
Ions moving slowly throughhigh pressure region
34
Why Tandem Mass Spectrometry?
• To separate the ionization step from the fragmentation step– for example, in an EI full scan mass spectrum of an analyte that
fragments extensively in the source, it can be difficult to determine which fragment ion is formed from which precursor – MS/MS allows individual ions to be selected and their fragmentation behavior studied in isolation from any other processes
• Direct mixture analysis
• Increase specificity, reduce “chemical noise” for quantitative studies (SRM/MRM)
35
Tandem Mass Spectrometry• In the simplest of these experiments, MS/MS, the 1st mass
analyzer is used to transmit only one ion observed (m2) in the full scan mass spectrum into the dissociation region
• In the dissociation region (collision cell), ions are “excited” energetically in a variety of fashions depending on the instrument type. This leads to the dissociation of m2 into fragment ions
• The 2nd mass analyzer is scanned to pass in turn the products of the dissociation of m2 onto the detector
• This is the simplest of the MS/MS experiments and is called a product ion scan
• There are many others: precursor ion scan, neutral loss scan, selected reaction monitoring
36
Tandem MS - Product Ion Scan Schematically
Full scan MS of analytem2
Mass select m2 and dissociateMS/MS spectra of m2
Mass select another ion (m3) from the MS/MS spectrum of m2 and dissociate
MS/MS/MS spectra or MS3
m3
37
Magnetic Sector Instruments• Ion dissociation in a Field Free Region (FFR):
– Metastable decomposition – Collision Induced Dissociation (CID)– Dissociation causes partitioning of ion kinetic energy and momentum
between the 2 particles
• Constant Linked scan with EB instruments:– To look at dissociations occurring in the 1st FFR– Must scan B/E together (linked) – Not true tandem MS because B and E are not operated separately– Poor precursor ion resolution
• Mass analyzed Ion Kinetic Energy Spectra (MIKES):– To look at dissociations occurring in the 2nd FFR– Only on BE instruments– Poor fragment ion resolution
38
Reminder: Metastable Ion (from section 3 (EI) pg7)
M+.
Fragment ions
Metastable ion
• M+. and fragment ions~0.3Dawide• Metastable ion~3Da wide!
39
Reminder: Metastable Ion (from section 3 (EI) pg7
• It’s position at m/z 200.3 can be used to determine which ion is fragmenting to givewhich product:For the reaction, M1
+ M2+ + M3
apparent mass of the metastable, M* = M22
____
M1• In this case, solving the equation: M1
+ is m/z 255 and M2+ is m/z 226
• Therefore this metastable ion corresponds to the fragmentation of the M+. ion to yield the fragment at m/z 226• the other metastable ion at m/z 146.6 corresponds to m/z 226 fragmenting to give 182
40
Magnetic Sector Instruments
• To overcome the resolution issues other sector based instruments have been built eg BEBE, EBEB etc
41
Product Ion Scan
Park Q1 to Allow Only Ions of a Single m/z ratio to pass into Q2
These ions collide with collision gas at a given CE and dissociate (CID)
Q3 is Scanned yielding the Full Scan Product Ion Spectra
Triple Quadrupole – MS/MS in Space
• Basic construction– QQQ configuration: Q1 and Q3 are mass filtering
with Q2 being the collision cell– Ar or N2 collision gas employed for MS/MS
Ion source DetectorQ1 Q2 Q3
42
QQQ – Full Scan Mass Spectrum
• Full scan mass spectrum of all source generated ions
Typical ESI Full Scan MS: Q3 scan, Q1 and Q2 Rf only mode
[M+H]+
little or no fragmentationobserved
Q1 Q2 Q3
Transmits all ions Transmits all ions Scan
43
QQQ – Product Ion Scan
• Full scan MS/MS spectrum of mass selected Parent Ion• Used for structural elucidation
Typical ESI Full Scan MS: Q3 scan, Q1 and Q2 Rf only mode
[M+H]+
little or no fragmentationobserved
Typical ESI Product Ion Scan:Q1 selects (M+H)+, CID occurs in Q2Q3 scanned
Q1 Q2 Q3
Selected Ion CID Scan
[M+H]+
44
Precursor Ion Scan
• Q3 is set to transmit only 1 ion characteristic of a specific class of compounds eg M1 = m/z 79 (PO3)-
• Then as species are introduced into the source, Q1 is scanned and only those compounds that fragment to yield M1 will be detected
• Used for target compound class detection usually with chromatography
Scan CID Selected Ion
Q1 Q2 Q3
45
Precursor Ion Scan
Time
Inte
nsit y
• β-Casein Digest Full scan• Complicated with many peptides
TimeIn
tens
i ty
Q3 monitoring only m/z 79
• β-Casein Digest Precursor Ion Scan• Detection of only Phosphorylated peptides
Courtesy of the MSCLS at the Univ. of Minn.
46
Neutral Loss Scan
Scan CID Scan at Q1-neutral mass
Q1 Q2 Q3
• Q1 and Q3 are both scanned however there is a mass offset (Mn) between Q1 and Q3
• Then as species are introduced into the source, only those compounds that loose the neutral mass, Mn, will be detected
• Used for target compound class detection usually with chromatography
47
Selected (Multiple) Reaction Monitoring –SRM/MRM
• From a complex mixture, Q1 is set to pass only the parent ion from a specific analyte, M1, and Q3 monitors only 1 of the unique fragment ions formed from M1
• Ideally this allows the unambiguous detection of only 1 (or more) analyte in a very complex mixture
• Used for target compound quantitation usually with chromatography
• The most sensitive and specific of all MS techniques for quantitation
Selected Ion CID Selected Fragment
Q1 Q2 Q3
48
3D Quadrupole Ion Trap – MS/MS in Time
Ring
Remember:
He buffer gas necessary for efficient trapping of ions directed into the ion trapHe present at all times therefore no delay between MS and MS/MS experiments
++
Endcap
Endcap
++
++
++
++
++
Ions gated into trap
detector
Courtesy of Agilent
49
QIT (ion isolation)
• An additional Rf voltage is applied to the end caps.• All but ions with one mass become non-stable and are
ejected from trap• Resonance excitation of the trapped ion with additional Rf
voltage → oscillations of trapped ion increases• The trapped ion collides with helium atoms and become
internally excited• Collision Induced Dissociation (CID)• New mass scan → MS/MS or (MS)3 spectrum• In analogy: (MS)3, (MS)4, ….
50
• 1: Clear Trap
• 2: Accumulation Time
• 3: Isolation Delay
• 4: Isolation begin
• 5: Fragmentation delay
• 6: Fragmentation begin*• 7: Scan delay
• 8: Mass Analysis**
QIT: MS/MS Scan
* ***
**
** **
Courtesy of Agilent
51
3D - QIT
• Can only perform product ion scans – no precursor, neutral loss or SRM functionality
• Most often used in qualitative analysis ie structural elucidation
• In scanning mode (MS, MS/MS), much more sensitive than a Q or QQQ
• MS/MSn
52
QQQ with Linear Ion Trap - QTrap
Q1 Q3Q0
N2 CAD Gas
Q2
linear ion trap3x10-5 Torr
Dipolar Aux AC
IQ1IQ2 IQ3
Exit
Skimmer
LINAC
courtesy of Applied Biosystems
53
Q-Trap• All the functionality of a QQQ
– Product ion Scan– Precursor Ion Scan– Neutral Loss Scan– SRM
• with the additional advantage that Q3 can be switched (software) into trapping mode operation
– Very high scanning sensitivity compared to Q operated with AC (Rf) and DC
– Linear trap also has some advantages over 3D QIT
• Can perform quantitation and structure elucidation (MS/MS3) sequentially in a chromatographic time frame
54
QQQ with Linear Ion Trap - QTrap
Q1 Q3Q0
N2 CAD Gas
Q2
linear ion trap
3x10-5 Torr
Dipolar Aux AC
IQ1IQ2 IQ3
Exit
Skimmer
LINAC
courtesy of Applied Biosystems
MS3 - Implementation• Precursor ion selection in Q1.• Fragmentation in Q2.• Trap products in Q3.• RF/DC isolation in Q3.• Single frequency excitation in Q3.• Mass scan.
55
Complementary MS/MS Approaches:•Tandem in Space: Triple Quads
•Poor scanning sensitivity•Great for quantitation (SRM/MRM)•Very selective scans•No low mass cut-off
•Tandem-in-Time: 3D Ion Traps•Very sensitive scanning•Only product ion scans - MSn
•Only scanning•Low mass cut-off!
•3D vs 2D (linear) Traps•Linear traps have higher charge capacity•No low mass cut-off•Linear traps restricted to MS3
56
Hybrid Quadrupole Time of Flight - QTof• a QQQ where Q3 has been replaced by a reflectron TOF MS• TOF used to acquire (accumulate) both MS and MS/MS spectra• TOF accepts ions in a “pulsed” mode from the continuous ion beam
passed to the pusher by the optics
Courtesy of Waters
57
Q-Tof• Advantages:
• High resolution (104) and accurate mass• good scan sensitivity• MS and Product Ion MS/MS
• Disadvantages:• historically, TOF instruments suffer from a “poor”
dynamic range compared to Q instruments – this is changing
• no Precursor Ion, Neutral Loss or SRM/MRM capability
58
+ve ESI - Peptide MS
m/z200 400 600 800 1000 1200 1400 1600
%
0
100 785.82
411.26203.05
149.02 355.07219.02 776.82
786.32
797.31
804.80
805.29815.79816.29816.79
1570.67834.77
Glu-Gly-Val-Asn-Asp-Asn-Glu-Glu-Gly-Phe-Phe-Ser-Ala-ArgE-G-V-N-D-N-E-E-G-F-F-S-A-R
mwt = 1569.67
[M+H]+
[M+2H] 2+
59
+ve ESI - Peptide MS/MS
m/z200 400 600 800 1000 1200 1400 1600
%
0
100 175.13
1570.80
684.37
316.18684.29333.20 497.24
1570.59684.41
1056.54
685.40813.47
813.38
1056.361039.53814.48
942.44
1570.511056.60
1057.56
1570.401057.63
1571.76
1571.87
1571.901572.81
1572.89
1573.89
m/z200 400 600 800 1000 1200 1400 1600
%
0
100 684.38
333.21187.08
240.15
480.29
337.18
382.20
497.22627.36498.21
787.86
787.83
685.39
685.43
740.30
788.35
813.45
1056.53942.44814.42
924.44
815.46
943.51
1056.57 1285.651171.57
1058.54
1172.561286.60
1286.711287.59
MS/MS of [M+H]+ CE = 85eV Ar
MS/MS of [M+2H]2+ CE = 35eV Ar
Doubly charged peptide ions yield more sequence ions than does the singly charged counterpart!
60
C
R1
H
H2N C N
H
C
R2O
H
C
O
N
H
C
R3
H
C
O
N
H
C
R4
H
COOH
a1 b1 c1 a2 b2 c2 a3 b3
z1
c3
y1x2 x1x3 y3 y2 z2z3
– If this charge is retained on the N terminal fragment, the ion is classed as either a, b or c
– If the charge is retained on the C terminal, the ion type is either x, y or z
– A subscript indicates the number of residues in the fragment
How Do Peptides Fragment?H+
61
+ve ESI - Peptide MS/MS Sequencing
m/z200 400 600 800 1000 1200 1400 1600
%
0
100 684.38
333.21187.08
240.15
480.29
337.18
382.20
497.22627.36498.21
787.86
787.83
685.39
685.43
740.30
788.35
813.45
1056.53942.44814.42
924.44
815.46
943.51
1056.57 1285.651171.57
1058.54
1172.561286.60
1286.711287.59
MS/MS of [M+2H]2+ CE = 35eV Ar
E--G--V--N--D--N--E--E--G--F--F--S--A--Ry1y2y3y4y5y6y8 y7y9y13 y12 y11 y10
b1 b2 b3 b4 b5 b6 b7 b8 b9 b13b12b11b10
y11y10
y9y8
y7
y6
y5
y3 y4b2
62
• Low Energy CID (10eV to 100eV)– collision induced dissociation in a QQQ, IT or QTof– a peptide carrying a positive charge fragments mainly along its
backbone, generating predominantly a, b and y ions– In addition, ions which have lost ammonia (-17 Da) denoted a*, b* and
y* and water (-18 Da) denoted a°, b° and y° are often observed– Satellite ions from side chain cleavage are not observed.
• High Energy CID (keV)– collision induced dissociation in a Tof-Tof or a magnetic deflection
instrument– All of the ion series described above are observed in high energy
collision spectra. Relative abundances are composition dependent.– Unlike low energy CID, ions do not readily lose ammonia or water.– In addition, side chain cleavages can be observed, so called d, v and w
cleavages
63
Others?
• Of course:• Orbitrap (linear trap – new type of 3D IT)• Tof-Tof• Linear trap-FTICR• Trap-Tof etc etc• Ion mobility coupled to other types of mass
spectrometer eg QTof where the collision cell has been changed to allow IMS to be performed as well as conventional MS/MS expts
1
• Every ionization technique exhibits a compound-dependent response – that is, the same amount injected of different analytes will give a different MS response
• In general, every aspect of the MS experiment can influence the response from the analyte
• Ionization method
• Type of MS
• Chromatographic method
• Detector system
• Therefore a careful calibration of the instruments response versus the sample concentration is a pre-requisite for reliable quantitation
• Most MS quantitation methods employ chromatography
Quantitation in GC-MS and LC-MS
2
Important Definitions• Limit of detection (LOD)
– How small an amount can you see? Usually this is defined as theamount that will give a S/N of about 3.
• Limit of quantitation (LOQ)– How small an amount can be quantitatively measured? Usually
significantly higher than the LOD.
• Sensitivity– What’s the response per unit of analyte?
• Specificity– Is the instrument response due only to the analyte? How well does
our analysis cope with interferences?
• Linearity– Over what range is the response linear?
3
Important Definitions• Calibration standards
– Prepared samples of known concentration for which corresponding responses can be obtained
– Peak Area is most often employed as the response for mass spectrometric assays however Peak Heights can also be used but introduce a source of error
• Standard or Calibration Curve– A series of standards covering the analyte concentration range
expected in the samples
– Mathematical function or equation describing the relationship between instrument/ionization method/detector response and concentration
• Principle– Mass spectrometric quantification can be done ONLY by reference to
standards (External or Internal)
4
Precision and Accuracy
..
.... ...
.. .
.
.
.
... ...
..
. .
.
..
... .
... ..
A
DC
B
A: Accurate and ImpreciseB: Accurate and PreciseC: Inaccurate and ImpreciseD: Inaccurate and Precise
Precision (reproducibility):GC-MS < 1%HPLC-MS (electrospray):
Quadrupole ~ 1-2 %Ion trap ~ 8 %
5
Quantitation in GC-MS and LC-MS• Calibration
– In general, the response of a mass spectrometer to a specific analyte will vary significantly with time
– Some of this variability can be directly attributable to parameters directly related to the ionization process and use of the MS as the detector however there are other sources of error:
• injection reproducibility when chromatography is employed
• Sample handling and preparation
• Why?– over time, MS performance will decrease as a result of detector aging
and source/ion optics becoming contaminated
– sample components causing ion suppression or isobaric interferences
– this causes systematic variation in response/unit of analyte injected
6
Quantitation in GC-MS and LC-MS
• Solution:– Quantitation calibration must be performed in real time to overcome
these issues
– 3 types of Calibration Methodologies:
• External Standard Calibration
• Standard Addition
• Internal Standard Calibration
7
Quantitation in GC-MS and LC-MS• External Standard:
– Construct a calibration curve by injecting a series of analyte standards and plotting response against concentration
– The samples are then analyzed and their response is compared to the standard analyte response to derive their concentration
• However:– Number of ions produced by a given analyte at a given concentration
varies with time therefore calibration curve less stable– How closely does the standard matrix resemble the sample matrix?– Did the MS response change between the analysis of the standards
and samples?– These issues as well as some preparation errors can be overcome by
using an internal standard method
8
Quantitation in GC-MS and LC-MS• Standard Addition:
– The unknown sample is divided in 2 portions and a known amount of the analyte is spiked into one portion
– Samples measured both before and after addition
– The spiked sample shows a larger response and the difference in response between the spiked and unspiked is due to the spike and provides a calibration point to determine the amount of analyte in the original sample
– Calculation of analyte concentration requires analysis of multiple samples of each analyte ie with and without standard added
• However:– A linear response is assumed when a 2 point determination is made,
that is, no calibration curve
9
Quantitation in GC-MS and LC-MS• Internal standards (ISTD):
– A known amount of a reference compound (the internal standard) is added to every sample
– If it is added before sample workup/extraction and if it has similar chemical properties to the analyte then it can be used to compensate for:
• differences in recovery during sample preparation (extraction)• Ion suppression by residual matrix components• Instrumental variability (injection volume etc)
– Chemically as similar as possible but not the analyte itself (obviously)– no co-elution with matrix components– However, we must have analyte free (blank) sample matrix to prepare
calibration curve and QC’s– Gives improved accuracy and precision because an internal
reference is in every sample and is the method of choice for MS quantitation
10
• Internal standard selection:– isotopically labeled species is best
(13C/15N>2H)>homologue>>analogue– Could use an isomer of the analyte but if the MS/MS behavior is similar to
the analyte then it must be chromatographically resolved from the analyte
– 13C or 15N labeled standards preferred
– Usually deuterated (2H ) standards are used as they are more available than 13C or 15N
– The label must not be able to be exchanged during the analysis ie 1H/2H exchange – we need stably labeled ISTD’s
– several isotopes to avoid overlap with isotopic peaks of unlabelled analyte >3 labels is optimum
– In multi-component assays, the ideal situation is to employ an internal standard for each analyte
Quantitation in GC-MS and LC-MS
11
Schematic Representation of a Typical Quantitative MS Procedure
SAMPLECRUDE
EXTRACTANALYTICAL
SAMPLE
1a. Add internal standard(s)1b. Homogenize1c. Extract analytes and ISTD’s
2a. Purify (chromatography, further extraction etc)2b. Concentrate if necessary2c. Derivatize if necessary
RATIO OF RESPONSES[ANALYTE(S) TO ISTD(S)]
QUANTITY OFANALYTE
IN SAMPLE
1 32
4
3. Mass Spectrometric measurementemploying SIM or SRM with GC/MS(MS)or LC/MS(MS)
4. Comparison with calibration curve
12
• Direct introduction:• Fast and simple• Dirty samples will require extensive cleanup to minimize suppression
and interference (keep in mind that choice of ionization methods differ in their susceptibility to these problems)
• Chromatography/MS:• Not so simple to develop/find a method and then you need to solve any
compatibility issues eg involatile buffers, ion pair reagents• Takes longer• Many problematic impurities can be separated from the analyte, eg salts
which interfere with ESI will elute in the void volume of a reverse phase column - less sample cleanup may be required
• Keep in mind that LC columns are not infinitely tolerant of “junk”, and are not cheap!
• We may want to compare to say, a HPLC run using UV detection• Adds the specificity of retention time to the analysis, essential if we are
using an internal standard of the same molecular weight
Quantitation: Sample Introdution
13
Which Ionization Technique to Chose?• Electrospray (ESI)
– little or no heat applied excellent for thermally labile molecules– polar (ionic) to relatively non-polar molecules– LC flow: <1 to ~1000µL/min– Most susceptable to matrix effects ie SUPPRESSION
• APCI & APPI– Heat applied to vapourize sample and mobile phase therefore not for
thermally labile molecules!– medium to low polararity analytes– LC flow: 100 – 2000µL/min– Less prone to matrix effects
• Which technique gives the best response (sensitivity) for your analyte?
14
Methomyl
ESI APCI APPI
m/z200 400 600 8000
10000
20000
30000
40000
50000
60000
70000
80000
90000Max: 206617
163.
116
5.1
185.
018
6.1
347.
134
8.1
[M+H]+= 163
m/z200 400 600 8000
10000
20000
30000
40000
50000
60000
70000
80000
90000Max: 95891
106.
116
3.1
164.
1
[M+H]+= 163
m/z200 400 600 8000
10000
20000
30000
40000
50000
60000
70000
80000
90000Max: 3663
163.
1[M+H]+= 163
courtesy of Agilent
15
• Full scan: – Extracted ion chromatogram– Specificity based on mass alone eg (M+H)+
– Poor sensitivity compared to SIM and SRM
• Selected Ion Monitoring (SIM)– Specificity based on mass alone– More sensitive than full scan as we are only monitoring a few ions
rather than the full mass range
• Optimum:– Selected reaction monitoring (SRM, MRM) in MS/MS with QQQ– Specificity based on mass and unique fragmentation– MS/MS with ion trap/QTof – no SRM mode– Significant reduction of chemical noise (less sample preparation)– Best S/N (sensitivity) of all
Quantitation in GC-MS and LC-MS
16
Full Scan vs SIM vs SRM
Same sample injected in differentMS modes - increased specificityand detectability!
17
Calibration Curve with Internal Std
Analyte amount
Peak AreaRatio
..
.
.
..
.Peak area Ratio = area of analyte response
area of ISTD response
Stds, samples,QC’s andblanks ran in same “batch”
• The “batch”:– Blanks, std curve (S1-S8), 2QC samples (QC1 and QC2), ½ of
the unknowns, 2QC samples (QC1 and QC3), ½ of the unknowns, 2QC samples (QC2 and QC3)
.QC1
QC2
QC3
18
Calibration Curve with Internal Standard• Blanks are very important:
– matrix blank: where matrix containing none of the analytes is extracted using the same sample preparation scheme
– Internal standard blank: to assess whether the ISTD causes a response in the analyte channel
– Solvent blank: does the solvent used to re-dissolve the extracted sample interfere
– in many cases interference determines limit of quantitation (LOQ) and not the absolute detectability (LOD)
• QC’s– Samples of known concentration extracted along with unknowns to
assess method performance
19
Calibration Curve – General form
Absolute SignalIntensityor PeakArea ratio
concentration or amount
saturation
Linear range
Noise level
.
..
.
..
..
chemical bkgdor memory
adsorption
Peak area Ratio = area of analyte responsearea of ISTD response
20
Linear Dynamic Range
• Some mass spectrometric methods are more linear than others:– EI has the greatest linearity, say 5 to 7 orders of magnitude
– ESI is probably the poorest exhibiting ~ 3 orders of magnitude
– APCI/APPI is a little better with ~ 4 orders of magnitude
– Trapping instruments tend to have lower dynamic range than Q type instruments because they fill up ie space charging
– TDC with MCP type detectors used in Tof instruments are usually limited to ~3 orders of magnitude, whereas electron multipliers are much better ~ 6
– Linear or Quadratic regression is used to “fit” the calibration curve
21
Ion Suppression• Suppression:
– Competition and interference with analyte ionization resulting in decreased number of [M+H]+ or [M-H]- ions
• Caused by salts that form adducts and clusters with analyte:– Strong bases in positive mode eg Triethylamine (TEA)
– Acids in negative mode eg Trifluoracetic acid (TFA)
– Non-volatile buffers (phosphate) and ion pair reagents
– Non-covalent dimers [2M+H]+, trimers....
– Metal ion complexes, e.g. [2M+Cu]+, Cu+ eg from LC equipment
– Other conatminants in the system eg PEG, platicizers, residual matrix species
– Coeluting analytes with different proton affinities that is, analytes that compete for protons
22
Ion Suppression: Solutions
• Dilute sample (1:10+) before or after sample preparation
• Select ISTD to coelute with analyte:
- to achieve similar matrix effect for analyte and ISTD (compensation)
- ideally the stable isotopically labeled analyte (2H, 13C, 15N)
- force chemical analogue into coelution with analyte
- individual ISTD for each analyte, if analytes are chromatographically resolved
• Modify LC mobile phase composition, change stationary phase or perform a more extensive sample clean-up
• In general, the more complex the sample, the more likely it is that chromatography will improve your quantitative method
• Try APCI (or APPI) instead of ESI (if analyte is thermally stable)
23
Hints on Method Development• Some form of sample preparation is critically important for rugged
and robust quantitative measurements:– Solvent (liquid/liquid) extraction
– Solid phase extraction
• Prepare (external) calibration standards in same matrix as samples
• Internal Standard should match analyte structure as closely as possible
- goal is coelution of ISTD and analyte
• Check mass spectrometric interference with coeluting compounds– interferences from analyte isotope peaks (eg Cl, Br, S)
– metabolites and their fragmentation to the analyte
• perform as much chromatography as is necessary
1
Ion Focusing• Confine ions from dispersive environments and focus them spatially,
temporally and/or energetically at a point in space or on a relevant detector to improve MS response
• We can focus ions because their energy and/or the momentum is changeable – remember charged particles in an electric field
• Ion optics need to be in a vacuum (greatest effect)
• Accomplished using electrostatic lenses (plates, orifices, grids) or multipolesplaced in or close to the ion beam to cause ions to be deflected/focused
• Lens stacks for fast moving ions– While a charged particle is in an electric field force acts upon it. The faster the
particle the smaller the accumulated impulse (rate of change of momentum = mΔv)
– These plates can be stacked with as many as 30 sets to effect efficient focusing – very complicated
• Simple lenses for slow moving ions – Einzel lens
2
Electrostatic lenses• Basic types
– Immersion/aperture lenses – lens stacks and grids (shown below)
– Unipotential lenses – Einzel lens
Ion Beam
• All lenses are convergent• Focal point is independent of m/z
3
Einzel lens
• used in Tof’s, quads, ion entrance optics• Focuses ions without changing the kinetic energy
4
Ion Focusing
With collisionalcooling
Without collisionalcooling
• quadrupoles (also hexapoles and octopoles) in Rf only mode ie no DC voltage (a=0) act as wide band pass filters for ions - very efficient especially at higher pressures
• Collisional cooling of ions traveling slowly through Rf only multipoles with some collision gas present reduces the axial motion of ions and therefore increases the mass resolution (used in QTof instruments)
5
Ion Detection
• The Faraday Cup:• The ion beam impacts the FC and deposit their charge – the
resulting current flowing away from the FC results in a voltage that can be measured
• Used rarely except in isotope ratio MS ie very accurate but not very sensitive
6
Discrete Dynode Electron Multiplier• When an energetic particle (a positive or negative ion) impinges on the
surface of a metal or semiconductor a number of 20 electrons are emitted from the surface
• The ease of such emission is determined by the electron work function (we) of the respective material eg BeCu alloy oxide (we = 2.4eV) and the velocity of the impacting particle
• The higher the velocity of the impacting particle and the lower the we
the larger the number of 20 electrons formed:– larger, slow moving ions will yield fewer 20 electrons than small, fast
moving ions which leads to high mass discrimination
– Can be solved by employing a post-acceleration conversion dynode (PACD)
7
Discrete Dynode Electron Multiplier - no PACD
• If an electrode opposite to the location of 10 emission is held at a more positive potential, then all emitted electrons will be accelerated towards and hit the surface where they in turn cause the release of even more electrons
• With 12 to 18 discrete dynode stages held at about 100V more positive potential allows the ion signal to be detected by a sensitive preamplifier
8
Discrete Dynode Electron Multiplier – no PACD
• Normally have a gain of 106 – 107 (when new)
• Have a lifetime or around 1 – 2 years before having to be replaced
• Must be kept at high vacuum as the emission layers can be harmed by oxygen
• over time and with use the first dynode surface becomes damaged and is therefore less efficient at releasing electrons iegain is reduced
• This can be compensated for to some extent by increasing the voltage difference between the discrete dynodes however eventually the multiplier must be replaced
9
Electron Multiplier with Post-Acceleration Conversion Dynode
(ion beam)Electron collector
Potential gradient
Further
Amplification
and recording
20 electrons Dynodes
• All ions are accelerated to high velocity by the Post-Acceleration Conversion Dynode• All ions release ~ the same number of 20 electrons therefore high mass discriminationgreatly reduced!
ConversionDynode
10
Channeltron Multiplier – continnuous dynode
• The inner surface is composed of a layer of silicon dioxide over a conductive layer of lead oxide
• This surface has sufficiently high resistance to withstand the ~1.5 to 2.5kV placed across the multiplier
• The high voltage drops continuously from the entrance to the exit of the tube• Gain of around 105 to 106
• Ages in a similar fashion to a discrete electron multiplier• An array of linear channeltron multipliers is called a microchannel plate (MCP) –
each multiplier is of the order of a few micrometers in size
11
Microchannel plate (MCP)
• Channels are inclined by some degrees from the perpendicular so that ions strike the inner surface and cause 20 electron emission
• Gain is only ~ 103 to 104 so sometimes 2 MCP’s are sandwiched together so that the small offset angle of the channels oppose each other to form what is called a chevron plate
Ions
12
Reflectron Tof Head
MCP
Tof Pusher
Courtesy of Waters/Micromass
13
Photomultiplier with Conversion Dynode
• The 20 electrons from the conversion dynode strike a phosphor which emits photons
• The photomultiplier detector has a much longer lifetime than an electron multiplier as it is a sealed device (under vacuum)
• 107 gain
14
• Advantages:– Long lifetime and gain does not decrease with time (compared with
an electron multiplier)
• Disadvantages:– dark current – when an intense signal ie many electrons strike the
phosphor it can take some time for the phosphor to stop releasing photons even when no electrons are hitting it
– Causes a signal to be recorded when there is no signal
Photomultiplier with Conversion Dynode
1
Ionization Technique Summary
Non-ionic organics<1,000stableLow to medAPCI/APPI
Polar/ionic organics, peptides, proteins, biomolecules, polymers, organometallics
<100,000labileMed to highESI
Peptides, proteins, RNA, DNA, polymers
<200,000labileMed to highMALDI
Polar/ionic organics, peptides, biomolecules, organometallics
<20,000labileMed to highFAB/LSIMS
Non-ionic organics, peptides, organometallics, carbohydrates
<2,000labileLow to medFD
Non-ionic organics<1,000stableLow to medFI
Non-ionic organics<1,000stableLowCI
Non-ionic organics<1,000stableLowEIExamplesMwtThermallyPolarityIonization
2
MS Experiment Summary
DIP (EI, CI, FAB/LSIMS and MALDI)Infusion (ESI and CF-FAB)
AllAllBatch Introduction
Q, QQQ, linear and 3D IT, Tof, QTof, FTICRMS
EB/BE, Q, QQQ, 3D-IT, Tof
QQQ, linear and 3D IT, QTof, and FTICRMS(other hybrids)
EB/BE, reflectron Tofand FTICRMS
Q, QQQ, EB/BE, linear and 3D IT, linear Tof
Instrument Type CommentIonization Experiment
Complex mixture analysis of more polar species
ESI, APCI, APPI
LC/MS
Complex mixture analysis of semi-volatile species
EI, CI, FIGC/MS
Structural elucidation and quantitation (SRM/MRM)
allMS/MS
Accurate mass yields elemental composition
EI, FAB/LSIMS,MALDI, ESI
High resn
Mass spectrum (some database searching capability for EI)
allLow resn
3
Mass Analyzers Summary
Unlimited (L)10,000 (R)
106
4,000
4,000
~15,000
MassRange
~1,000 (L)Up to 20,000 (R)
allpulsedTOF
105 to 106EI, CI, ESI, APCI, APPI, MALDI
pulsedFTICRMS
~3,000EI, CI, ESI, APCI, APPI, AP-MALDI
pulsedIon Trap(linear and 3D)
Normally 3,000but 10,000possible
EI, CI, ESI, APCI, APPI
continuousQuadrupole(Q and QQQ)
Variable upto 100,000
EI, CI,FAB/LSIMS
continuousSector(BE/EB)
ResolutionIonizationModes
IonDetection
Analyzer
L = Linear Tof and R = Reflectron Tof