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7/29/2019 Mossbauer spectra
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Mssbauer spectroscopy
A Mssbauer absorption spectrum of57Fe
Mssbauer spectroscopy is a spectroscopictechnique based on the Mssbauer effect. Thiseffect, discovered by Rudolf Mssbauerin 1957, consists of the recoil-free, resonant absorption
and emission ofgamma raysin solids.
LikeNMR spectroscopy, Mssbauer spectroscopy probes tiny changes in the energy levels of an
atomic nucleus in response to its environment. Typically, three types ofnuclear interaction maybe observed: an isomer shift, also known as achemical shift;quadrupole splitting; and magnetic
orhyperfine splitting, also known as the Zeeman effect. Due to the high energy and extremely
narrow line widths of gamma rays, Mssbauer spectroscopy is a very sensitive technique interms of energy (and hence frequency) resolution, capable of detecting change in just a few parts
per 1011.
Basic principle
Just as a gun recoils when a bullet is fired, conservation of momentum requires a free nucleus(such as in a gas) to recoil during emission or absorption of a gamma ray. If a nucleus at rest
emits a gamma ray, the energy of the gamma ray is slightly less than the natural energy of the
transition, but in order for a nucleus at rest to absorb a gamma ray, the gamma ray's energy mustbe slightly greater than the natural energy, because in both cases energy is lost to recoil. This
means that nuclear resonance (emission and absorption of the same gamma ray) is unobservable
with free nuclei, because the shift in energy is too great and the emission and absorption spectra
have no significant overlap.
Nuclei in a solid crystal, however, are not free to recoil because they are bound in place in the
crystal lattice. When a nucleus in a solid emits or absorbs a gamma ray, some energy can still be
lost as recoil energy, but in this case it always occurs in discrete packets called phonons
(quantized vibrations of the crystal lattice). Any whole number of phonons can be emitted,including zero, which is known as a "recoil-free" event. In this case conservation of momentum
is satisfied by the momentum of the crystal as a whole, so practically no energy is lost.
http://en.wikipedia.org/wiki/File:Mossbauer_51Fe.pnghttp://en.wikipedia.org/wiki/Spectroscopyhttp://en.wikipedia.org/wiki/Spectroscopyhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_effecthttp://en.wikipedia.org/wiki/Rudolf_M%C3%B6ssbauerhttp://en.wikipedia.org/wiki/Rudolf_M%C3%B6ssbauerhttp://en.wikipedia.org/wiki/Gamma_rayhttp://en.wikipedia.org/wiki/Gamma_rayhttp://en.wikipedia.org/wiki/Solidhttp://en.wikipedia.org/wiki/NMR_spectroscopyhttp://en.wikipedia.org/wiki/Nuclear_interactionhttp://en.wikipedia.org/wiki/Isomer_shifthttp://en.wikipedia.org/wiki/Isomer_shifthttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/Zeeman_effecthttp://en.wikipedia.org/wiki/Spectral_linehttp://en.wikipedia.org/wiki/Conservation_of_momentumhttp://en.wikipedia.org/wiki/Crystalhttp://en.wikipedia.org/wiki/Phononhttp://en.wikipedia.org/wiki/File:Mossbauer_51Fe.pnghttp://en.wikipedia.org/wiki/File:Mossbauer_51Fe.pnghttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_effecthttp://en.wikipedia.org/wiki/Rudolf_M%C3%B6ssbauerhttp://en.wikipedia.org/wiki/Gamma_rayhttp://en.wikipedia.org/wiki/Solidhttp://en.wikipedia.org/wiki/NMR_spectroscopyhttp://en.wikipedia.org/wiki/Nuclear_interactionhttp://en.wikipedia.org/wiki/Isomer_shifthttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/Zeeman_effecthttp://en.wikipedia.org/wiki/Spectral_linehttp://en.wikipedia.org/wiki/Conservation_of_momentumhttp://en.wikipedia.org/wiki/Crystalhttp://en.wikipedia.org/wiki/Phononhttp://en.wikipedia.org/wiki/Spectroscopy7/29/2019 Mossbauer spectra
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As an analogy, imagine jumping from a boat to shore, and imagine that the distance from the
boat to shore is the longest you can possibly jump (on land). If the boat is floating in water, you
will fall short because some of your energy goes into pushing the boat back. If the water isfrozen solid, however, you will be able to make it.
Mssbauer found that a significant fraction of emission and absorption events will be recoil-free,which is quantified using the LambMssbauer factor.[2] This fact is what makes Mssbauer
spectroscopy possible, because it means gamma rays emitted by one nucleus can be resonantlyabsorbed by a sample containing nuclei of the same isotope, and this absorption can be
measured.
Typical method
In its most common form, Mssbauer absorption spectroscopy, a solid sample is exposed to abeam ofgamma radiation, and a detector measures the intensity of the beam transmitted through
the sample. The atoms in the source emitting the gamma rays must be of the same isotope as the
atoms in the sample absorbing them.
If the emitting and absorbing nuclei were in identical chemical environments, the nucleartransition energies would be exactly equal and resonant absorption would be observed with both
materials at rest. The difference in chemical environments, however, causes the nuclear energy
levels to shift in a few different ways, as described below. Although these energy shifts are tiny(often less than a micro-electronvolt), the extremely narrow spectral linewidthsof gamma rays
for some radionuclides make the small energy shifts correspond to large changes in absorbance.
To bring the two nuclei back into resonance it is necessary to change the energy of the gammaray slightly, and in practice this is always done using theDoppler effect.
During Mssbauer absorption spectroscopy, the source is accelerated through a range ofvelocities using a linear motor to produce a Doppler effect and scan the gamma ray energy
through a given range. A typical range of velocities for57Fe, for example, may be 11 mm/s(1 mm/s = 48.075 neV).
In the resulting spectra, gamma ray intensity is plotted as a function of the source velocity. At
velocities corresponding to the resonant energy levels of the sample, a fraction of the gamma
rays are absorbed, resulting in a drop in the measured intensity and a corresponding dip in thespectrum. The number, positions, and intensities of the dips (also called peaks; dips in
transmitted intensity are peaks in absorbance) provide information about the chemical
environment of the absorbing nuclei and can be used to characterize the sample.
Selecting a suitable source
Mssbauer spectroscopy is limited by the need for a suitable gamma-ray source. Usually, thisconsists of a radioactive parent that decays to the desired isotope. For example, the source for57Fe consists of57Co, which decays by electron capture to anexcited state of57Fe, then
subsequently decays to a ground state emitting the desired gamma-ray. The radioactive cobalt isprepared on a foil, often of rhodium.[4] Ideally theparent isotope will have a sufficiently long
http://en.wikipedia.org/wiki/Lamb%E2%80%93M%C3%B6ssbauer_factorhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-G.C3.BCtlich-2http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-G.C3.BCtlich-2http://en.wikipedia.org/wiki/Gamma_rayhttp://en.wikipedia.org/wiki/Electronvolthttp://en.wikipedia.org/wiki/Spectral_linewidthhttp://en.wikipedia.org/wiki/Spectral_linewidthhttp://en.wikipedia.org/wiki/Absorbancehttp://en.wikipedia.org/wiki/Doppler_effecthttp://en.wikipedia.org/wiki/Doppler_effecthttp://en.wikipedia.org/wiki/Doppler_effecthttp://en.wikipedia.org/wiki/Linear_motorhttp://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Cobalt-57http://en.wikipedia.org/wiki/Cobalt-57http://en.wikipedia.org/wiki/Electron_capturehttp://en.wikipedia.org/wiki/Excited_statehttp://en.wikipedia.org/wiki/Excited_statehttp://en.wikipedia.org/wiki/Ground_statehttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-4http://en.wikipedia.org/wiki/Parenthttp://en.wikipedia.org/wiki/Lamb%E2%80%93M%C3%B6ssbauer_factorhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-G.C3.BCtlich-2http://en.wikipedia.org/wiki/Gamma_rayhttp://en.wikipedia.org/wiki/Electronvolthttp://en.wikipedia.org/wiki/Spectral_linewidthhttp://en.wikipedia.org/wiki/Absorbancehttp://en.wikipedia.org/wiki/Doppler_effecthttp://en.wikipedia.org/wiki/Linear_motorhttp://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Cobalt-57http://en.wikipedia.org/wiki/Electron_capturehttp://en.wikipedia.org/wiki/Excited_statehttp://en.wikipedia.org/wiki/Ground_statehttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-4http://en.wikipedia.org/wiki/Parent7/29/2019 Mossbauer spectra
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half-life to remain useful, but will also have a sufficient decay rate to supply the required
intensity of radiation. Also, the gamma-ray energy should be relatively low, otherwise the system
will have a low recoil-free fraction resulting in a poorsignal-to-noise ratio and requiring longcollection times. The periodic table below indicates those elements having an isotope suitable for
Mssbauer spectroscopy. Of these,57Fe is by far the most common element studied using the
technique, although129
I,119
Sn, and121
Sb are also frequently studied.
[hide]
Periodic table of Mssbauer active elements
H He
Li Be B C N O F Ne
Na Mg Al Si P S Cl Ar
K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr
Rb Sr Y ZrNb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe
Cs Ba La Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn
Fr Ra Ac Rf Db Sg Bh Hs Mt Ds Rg Cn Uut Fl Uup Lv Uus Uuo
Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr
Mssbauer-active elements Gamma-ray sources Unsuitable for Mssbauer
Analysis of Mssbauer spectra
As described above, Mssbauer spectroscopy has an extremely fine energy resolution and candetect even subtle changes in the nuclear environment of the relevant atoms. Typically, there are
three types ofnuclear interactions that are observed, isomer shift (orchemical shift), quadrupole
splitting and hyperfine splitting (orZeeman splitting).[5][6]
Isomer shift () is a relative measure describing a shift in the resonance energy of a nucleus due
to the transition of electrons within itss orbital. The whole spectrum is shifted in either a positive
or negative direction depending upon the s electron charge density. This change arises due to
alterations in the electrostatic response between the non-zero probability s orbital electrons andthe non-zero volume nucleus they orbit.
Only electrons in s orbitals demonstrate non-zero probability because their 3D spherical shape
incorporates the volume taken up by the nucleus. However, the p, d, and other electrons may
influence the s electron density through a screening effect. The s electron density can also beaffected by the oxidation state and the chemical environment of the atom.
Isomer shift (chemical shift, CS) can be expressed using the formula below, where K is a nuclear
constant, the difference between Re2 and Rg
2 is the effective nuclear charge radius differencebetween excited state and the ground state, and the difference between [s
2(0)]a and [s2(0)]b is
the electron density difference on the nucleus (a = source, b = sample). Isomer shift does not
http://en.wikipedia.org/wiki/Signal-to-noise_ratiohttp://en.wikipedia.org/wiki/Signal-to-noise_ratiohttp://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iodine-129http://en.wikipedia.org/wiki/Iodine-129http://en.wikipedia.org/wiki/Tin-119http://en.wikipedia.org/wiki/Tin-119http://en.wikipedia.org/wiki/Tin-119http://en.wikipedia.org/wiki/Antimony-121http://en.wikipedia.org/wiki/Antimony-121http://en.wikipedia.org/wiki/Antimony-121http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopyhttp://en.wikipedia.org/wiki/Periodic_tablehttp://en.wikipedia.org/wiki/Hydrogenhttp://en.wikipedia.org/wiki/Heliumhttp://en.wikipedia.org/wiki/Lithiumhttp://en.wikipedia.org/wiki/Berylliumhttp://en.wikipedia.org/wiki/Boronhttp://en.wikipedia.org/wiki/Carbonhttp://en.wikipedia.org/wiki/Nitrogenhttp://en.wikipedia.org/wiki/Oxygenhttp://en.wikipedia.org/wiki/Fluorinehttp://en.wikipedia.org/wiki/Neonhttp://en.wikipedia.org/wiki/Sodiumhttp://en.wikipedia.org/wiki/Magnesiumhttp://en.wikipedia.org/wiki/Aluminiumhttp://en.wikipedia.org/wiki/Siliconhttp://en.wikipedia.org/wiki/Phosphorushttp://en.wikipedia.org/wiki/Sulfurhttp://en.wikipedia.org/wiki/Chlorinehttp://en.wikipedia.org/wiki/Argonhttp://en.wikipedia.org/wiki/Potassiumhttp://en.wikipedia.org/wiki/Calciumhttp://en.wikipedia.org/wiki/Scandiumhttp://en.wikipedia.org/wiki/Titaniumhttp://en.wikipedia.org/wiki/Vanadiumhttp://en.wikipedia.org/wiki/Chromiumhttp://en.wikipedia.org/wiki/Manganesehttp://en.wikipedia.org/wiki/Ironhttp://en.wikipedia.org/wiki/Cobalthttp://en.wikipedia.org/wiki/Nickelhttp://en.wikipedia.org/wiki/Copperhttp://en.wikipedia.org/wiki/Zinchttp://en.wikipedia.org/wiki/Galliumhttp://en.wikipedia.org/wiki/Germaniumhttp://en.wikipedia.org/wiki/Arsenichttp://en.wikipedia.org/wiki/Seleniumhttp://en.wikipedia.org/wiki/Brominehttp://en.wikipedia.org/wiki/Kryptonhttp://en.wikipedia.org/wiki/Rubidiumhttp://en.wikipedia.org/wiki/Strontiumhttp://en.wikipedia.org/wiki/Yttriumhttp://en.wikipedia.org/wiki/Zirconiumhttp://en.wikipedia.org/wiki/Niobiumhttp://en.wikipedia.org/wiki/Molybdenumhttp://en.wikipedia.org/wiki/Technetiumhttp://en.wikipedia.org/wiki/Rutheniumhttp://en.wikipedia.org/wiki/Rhodiumhttp://en.wikipedia.org/wiki/Palladiumhttp://en.wikipedia.org/wiki/Silverhttp://en.wikipedia.org/wiki/Cadmiumhttp://en.wikipedia.org/wiki/Indiumhttp://en.wikipedia.org/wiki/Tinhttp://en.wikipedia.org/wiki/Antimonyhttp://en.wikipedia.org/wiki/Telluriumhttp://en.wikipedia.org/wiki/Iodinehttp://en.wikipedia.org/wiki/Xenonhttp://en.wikipedia.org/wiki/Caesiumhttp://en.wikipedia.org/wiki/Bariumhttp://en.wikipedia.org/wiki/Lanthanumhttp://en.wikipedia.org/wiki/Hafniumhttp://en.wikipedia.org/wiki/Tantalumhttp://en.wikipedia.org/wiki/Tungstenhttp://en.wikipedia.org/wiki/Rheniumhttp://en.wikipedia.org/wiki/Osmiumhttp://en.wikipedia.org/wiki/Iridiumhttp://en.wikipedia.org/wiki/Platinumhttp://en.wikipedia.org/wiki/Goldhttp://en.wikipedia.org/wiki/Mercury_(element)http://en.wikipedia.org/wiki/Thalliumhttp://en.wikipedia.org/wiki/Leadhttp://en.wikipedia.org/wiki/Bismuthhttp://en.wikipedia.org/wiki/Poloniumhttp://en.wikipedia.org/wiki/Astatinehttp://en.wikipedia.org/wiki/Radonhttp://en.wikipedia.org/wiki/Franciumhttp://en.wikipedia.org/wiki/Radiumhttp://en.wikipedia.org/wiki/Actiniumhttp://en.wikipedia.org/wiki/Rutherfordiumhttp://en.wikipedia.org/wiki/Dubniumhttp://en.wikipedia.org/wiki/Seaborgiumhttp://en.wikipedia.org/wiki/Bohriumhttp://en.wikipedia.org/wiki/Hassiumhttp://en.wikipedia.org/wiki/Meitneriumhttp://en.wikipedia.org/wiki/Darmstadtiumhttp://en.wikipedia.org/wiki/Roentgeniumhttp://en.wikipedia.org/wiki/Coperniciumhttp://en.wikipedia.org/wiki/Ununtriumhttp://en.wikipedia.org/wiki/Fleroviumhttp://en.wikipedia.org/wiki/Ununpentiumhttp://en.wikipedia.org/wiki/Livermoriumhttp://en.wikipedia.org/wiki/Ununseptiumhttp://en.wikipedia.org/wiki/Ununoctiumhttp://en.wikipedia.org/wiki/Ceriumhttp://en.wikipedia.org/wiki/Praseodymiumhttp://en.wikipedia.org/wiki/Neodymiumhttp://en.wikipedia.org/wiki/Promethiumhttp://en.wikipedia.org/wiki/Samariumhttp://en.wikipedia.org/wiki/Europiumhttp://en.wikipedia.org/wiki/Gadoliniumhttp://en.wikipedia.org/wiki/Terbiumhttp://en.wikipedia.org/wiki/Dysprosiumhttp://en.wikipedia.org/wiki/Holmiumhttp://en.wikipedia.org/wiki/Erbiumhttp://en.wikipedia.org/wiki/Thuliumhttp://en.wikipedia.org/wiki/Ytterbiumhttp://en.wikipedia.org/wiki/Lutetiumhttp://en.wikipedia.org/wiki/Thoriumhttp://en.wikipedia.org/wiki/Protactiniumhttp://en.wikipedia.org/wiki/Uraniumhttp://en.wikipedia.org/wiki/Neptuniumhttp://en.wikipedia.org/wiki/Plutoniumhttp://en.wikipedia.org/wiki/Americiumhttp://en.wikipedia.org/wiki/Curiumhttp://en.wikipedia.org/wiki/Berkeliumhttp://en.wikipedia.org/wiki/Californiumhttp://en.wikipedia.org/wiki/Einsteiniumhttp://en.wikipedia.org/wiki/Fermiumhttp://en.wikipedia.org/wiki/Mendeleviumhttp://en.wikipedia.org/wiki/Nobeliumhttp://en.wikipedia.org/wiki/Lawrenciumhttp://en.wikipedia.org/wiki/Nuclear_interactionhttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/Zeeman_splittinghttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-RSC2-5http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-G.C3.BCtlich_et_al-6http://en.wikipedia.org/wiki/Screening_effecthttp://en.wikipedia.org/wiki/Screening_effecthttp://en.wikipedia.org/wiki/Isomer_shifthttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Signal-to-noise_ratiohttp://en.wikipedia.org/wiki/Iron-57http://en.wikipedia.org/wiki/Iodine-129http://en.wikipedia.org/wiki/Tin-119http://en.wikipedia.org/wiki/Antimony-121http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopyhttp://en.wikipedia.org/wiki/Periodic_tablehttp://en.wikipedia.org/wiki/Hydrogenhttp://en.wikipedia.org/wiki/Heliumhttp://en.wikipedia.org/wiki/Lithiumhttp://en.wikipedia.org/wiki/Berylliumhttp://en.wikipedia.org/wiki/Boronhttp://en.wikipedia.org/wiki/Carbonhttp://en.wikipedia.org/wiki/Nitrogenhttp://en.wikipedia.org/wiki/Oxygenhttp://en.wikipedia.org/wiki/Fluorinehttp://en.wikipedia.org/wiki/Neonhttp://en.wikipedia.org/wiki/Sodiumhttp://en.wikipedia.org/wiki/Magnesiumhttp://en.wikipedia.org/wiki/Aluminiumhttp://en.wikipedia.org/wiki/Siliconhttp://en.wikipedia.org/wiki/Phosphorushttp://en.wikipedia.org/wiki/Sulfurhttp://en.wikipedia.org/wiki/Chlorinehttp://en.wikipedia.org/wiki/Argonhttp://en.wikipedia.org/wiki/Potassiumhttp://en.wikipedia.org/wiki/Calciumhttp://en.wikipedia.org/wiki/Scandiumhttp://en.wikipedia.org/wiki/Titaniumhttp://en.wikipedia.org/wiki/Vanadiumhttp://en.wikipedia.org/wiki/Chromiumhttp://en.wikipedia.org/wiki/Manganesehttp://en.wikipedia.org/wiki/Ironhttp://en.wikipedia.org/wiki/Cobalthttp://en.wikipedia.org/wiki/Nickelhttp://en.wikipedia.org/wiki/Copperhttp://en.wikipedia.org/wiki/Zinchttp://en.wikipedia.org/wiki/Galliumhttp://en.wikipedia.org/wiki/Germaniumhttp://en.wikipedia.org/wiki/Arsenichttp://en.wikipedia.org/wiki/Seleniumhttp://en.wikipedia.org/wiki/Brominehttp://en.wikipedia.org/wiki/Kryptonhttp://en.wikipedia.org/wiki/Rubidiumhttp://en.wikipedia.org/wiki/Strontiumhttp://en.wikipedia.org/wiki/Yttriumhttp://en.wikipedia.org/wiki/Zirconiumhttp://en.wikipedia.org/wiki/Niobiumhttp://en.wikipedia.org/wiki/Molybdenumhttp://en.wikipedia.org/wiki/Technetiumhttp://en.wikipedia.org/wiki/Rutheniumhttp://en.wikipedia.org/wiki/Rhodiumhttp://en.wikipedia.org/wiki/Palladiumhttp://en.wikipedia.org/wiki/Silverhttp://en.wikipedia.org/wiki/Cadmiumhttp://en.wikipedia.org/wiki/Indiumhttp://en.wikipedia.org/wiki/Tinhttp://en.wikipedia.org/wiki/Antimonyhttp://en.wikipedia.org/wiki/Telluriumhttp://en.wikipedia.org/wiki/Iodinehttp://en.wikipedia.org/wiki/Xenonhttp://en.wikipedia.org/wiki/Caesiumhttp://en.wikipedia.org/wiki/Bariumhttp://en.wikipedia.org/wiki/Lanthanumhttp://en.wikipedia.org/wiki/Hafniumhttp://en.wikipedia.org/wiki/Tantalumhttp://en.wikipedia.org/wiki/Tungstenhttp://en.wikipedia.org/wiki/Rheniumhttp://en.wikipedia.org/wiki/Osmiumhttp://en.wikipedia.org/wiki/Iridiumhttp://en.wikipedia.org/wiki/Platinumhttp://en.wikipedia.org/wiki/Goldhttp://en.wikipedia.org/wiki/Mercury_(element)http://en.wikipedia.org/wiki/Thalliumhttp://en.wikipedia.org/wiki/Leadhttp://en.wikipedia.org/wiki/Bismuthhttp://en.wikipedia.org/wiki/Poloniumhttp://en.wikipedia.org/wiki/Astatinehttp://en.wikipedia.org/wiki/Radonhttp://en.wikipedia.org/wiki/Franciumhttp://en.wikipedia.org/wiki/Radiumhttp://en.wikipedia.org/wiki/Actiniumhttp://en.wikipedia.org/wiki/Rutherfordiumhttp://en.wikipedia.org/wiki/Dubniumhttp://en.wikipedia.org/wiki/Seaborgiumhttp://en.wikipedia.org/wiki/Bohriumhttp://en.wikipedia.org/wiki/Hassiumhttp://en.wikipedia.org/wiki/Meitneriumhttp://en.wikipedia.org/wiki/Darmstadtiumhttp://en.wikipedia.org/wiki/Roentgeniumhttp://en.wikipedia.org/wiki/Coperniciumhttp://en.wikipedia.org/wiki/Ununtriumhttp://en.wikipedia.org/wiki/Fleroviumhttp://en.wikipedia.org/wiki/Ununpentiumhttp://en.wikipedia.org/wiki/Livermoriumhttp://en.wikipedia.org/wiki/Ununseptiumhttp://en.wikipedia.org/wiki/Ununoctiumhttp://en.wikipedia.org/wiki/Ceriumhttp://en.wikipedia.org/wiki/Praseodymiumhttp://en.wikipedia.org/wiki/Neodymiumhttp://en.wikipedia.org/wiki/Promethiumhttp://en.wikipedia.org/wiki/Samariumhttp://en.wikipedia.org/wiki/Europiumhttp://en.wikipedia.org/wiki/Gadoliniumhttp://en.wikipedia.org/wiki/Terbiumhttp://en.wikipedia.org/wiki/Dysprosiumhttp://en.wikipedia.org/wiki/Holmiumhttp://en.wikipedia.org/wiki/Erbiumhttp://en.wikipedia.org/wiki/Thuliumhttp://en.wikipedia.org/wiki/Ytterbiumhttp://en.wikipedia.org/wiki/Lutetiumhttp://en.wikipedia.org/wiki/Thoriumhttp://en.wikipedia.org/wiki/Protactiniumhttp://en.wikipedia.org/wiki/Uraniumhttp://en.wikipedia.org/wiki/Neptuniumhttp://en.wikipedia.org/wiki/Plutoniumhttp://en.wikipedia.org/wiki/Americiumhttp://en.wikipedia.org/wiki/Curiumhttp://en.wikipedia.org/wiki/Berkeliumhttp://en.wikipedia.org/wiki/Californiumhttp://en.wikipedia.org/wiki/Einsteiniumhttp://en.wikipedia.org/wiki/Fermiumhttp://en.wikipedia.org/wiki/Mendeleviumhttp://en.wikipedia.org/wiki/Nobeliumhttp://en.wikipedia.org/wiki/Lawrenciumhttp://en.wikipedia.org/wiki/Nuclear_interactionhttp://en.wikipedia.org/wiki/Chemical_shifthttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Quadrupole_splittinghttp://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/Zeeman_splittinghttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-RSC2-5http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-G.C3.BCtlich_et_al-6http://en.wikipedia.org/wiki/Screening_effecthttp://en.wikipedia.org/wiki/Isomer_shifthttp://en.wikipedia.org/wiki/Chemical_shift7/29/2019 Mossbauer spectra
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change with temperature, however, a small changes are generally attributed to second-order
Doppler effect.
CS = K (Re2 Rg
2) {[s2(0)]a [s
2(0)]b}
Chemical shift and quadrupole splitting of the nuclear energy levels and correspondingMssbauer spectra
The physical meaning of this equation can be clarified using examples:
1. While an increase ins electron density in 57Fe spectrum gives a negative shift because the
change in the effective nuclear charge is negative, an increase in s electron density in119Sn gives a positive shift due to a positive change in overall nuclear charge.
2. Oxidised ferric ions (Fe3+) have lower isomer shifts than ferrous ions (Fe2+) because s
electron density at the nucleus of ferric ions is greater due to a weaker screening effect by
delectrons.[7]
Quadrupole Splitting reflects the interaction between the nuclear energy levels and surrounding
electric field gradient (EFG). Nuclei in states with non-spherical charge distributions, i.e. all
those with angular quantum number (I) greater than 1/2, produce an asymmetrical electric field
which splits the nuclear energy levels. This produces a nuclear quadrupole moment.[5]
In the case of an isotope with a I=3/2 excited state, such as 57Fe or119Sn, the 3/2 to 1/2 transition
is split into two substates mI=1/2 and mI=3/2. These appear as two specific peaks in a
spectrum, sometimes referred to as a 'doublet'. Quadrupole splitting is measured as the separationbetween these two peaks and reflects the character of the electric field at the nucleus.
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Magnetic splitting of the nuclear energy levels and the corresponding Mssbauer spectrum
Magnetic splitting (hyperfine splitting) is a result of the interaction between the nucleus any
surrounding magnetic field. A nucleus with spin, I, splits into 2I + 1 sub-energy levels in thepresence of magnetic field. For example, a nucleus with spin state I= 3/2 will split into 4 non-
degenerate sub-states with mI values of +3/2, +1/2, -1/2 and 3/2. Each split is hyperfine, being
in the order of 107eV. The restriction rule of magnetic dipoles means that transitions between
the excited state and ground state can only occur where m I changes by 0 or 1. This gives sixpossible transitions for a 3/2 to 1/2 transition.[5] Generally speaking therefore, in the majority of
cases only six peaks can be monitored in a spectrum produced by a hyperfine splitting nucleus.
The three Mssbauer parameters: isomer shift, quadrupole splitting, and hyperfine splitting can
often be used to identify a particular compound by comparing it to known spectra. A largedatabase including most of the published Mssbauer parameters available in the literature is
maintained by the Mssbauer Effect Data Center.[8]In some cases, a compound may have more
than one possible position for the Mssbauer active atom. For example, the crystal structure ofmagnetite (Fe3O4) supports two unique sites for the iron atoms. The corresponding spectrum
therefore has twelve peaks, a 'hextet' for each potential atomic site. Thus, magnetite also has two
sets of Mssbauer parameters, one for each site.
Combination of all: Many times it is very common to observe all effects-isomer shift,
quadrupole splitting and magnetic Zeeman effect- in a spectrum. In such cases the isomer shift is
given by the average of all lines. The quadrupole splitting when all the four excited substates are
equally shifted (two substates are lifted and other two are lowered) is given the shift of the outertwo lines relative to the inner two lines (generally innermost two lines are not considered). If the
shifting of four substates are not equal then the quadrupole splitting is often extracted using
fitting software where all the six lines are taken in to account.
In addition, the relative intensities of the various peaks reflect the relative concentrations ofcompounds in a sample and can be used for semi-quantitative analysis. Also, since ferromagnetic
http://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-RSC2-5http://en.wikipedia.org/w/index.php?title=M%C3%B6ssbauer_Effect_Data_Center&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=M%C3%B6ssbauer_Effect_Data_Center&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-8http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-8http://en.wikipedia.org/wiki/Magnetitehttp://en.wikipedia.org/wiki/Magnetitehttp://en.wikipedia.org/wiki/File:Mossbauer_-Magnetting_Splitting.jpghttp://en.wikipedia.org/wiki/File:Mossbauer_-Magnetting_Splitting.jpghttp://en.wikipedia.org/wiki/Hyperfine_splittinghttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-RSC2-5http://en.wikipedia.org/w/index.php?title=M%C3%B6ssbauer_Effect_Data_Center&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-8http://en.wikipedia.org/wiki/Magnetite7/29/2019 Mossbauer spectra
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phenomena are size-dependent, in some cases spectra can provide insight into the crystallite size
and grain structure of a material.
Applications of Mssbauer spectroscopy
Among the drawbacks of the technique are the limited number of gamma ray sources and therequirement that samples be solid in order to eliminate the recoil of the nucleus. Mssbauer
spectroscopy is unique in its sensitivity to subtle changes in the chemical environment of the
nucleus including oxidation state changes, the effect of different ligands on a particular atom,and the magnetic environment of the sample.
As an analytical tool Mssbauer spectroscopy offers detection limits in the order of billionths of
an electron volt.It has been especially useful in the field of geology for identifying the
composition of iron-containing specimens including meteors and moon rocks. In situ datacollection of Mssbauer spectra has also been carried out on iron rich rocks on Mars.[9]
Another significant application of Mssbauer spectroscopy is the study of phase transformationsthat occur in iron catalysts during FischerTropsch synthesis. While these catalysts initially
consist of hematite (Fe2O3), during reaction they are transformed into a mixture of magnetite(Fe3O4) and several iron carbides. The formation of carbides appears to improve catalytic
activity, however it can also lead to the mechanical break-up and attrition of the catalyst
particles. This can cause difficulties in the final separation of catalyst from reaction products.[10]
Mssbauer spectroscopy has also been used to determine the relative concentration change in theoxidation state of antimony (Sb) during the selective oxidation ofolefins. During calcinationall
the Sb ions in an antimony-containing tin dioxide catalyst transform into the +5 oxidation state.
Following the catalytic reaction, almost all Sb ions revert from the +5 to the +3 oxidation state.
A significant change in the chemical environment surrounding the antimony nucleus occursduring the oxidation state change which can easily be monitored as an isomer shift in the
Mssbauer spectrum.[11]
This technique has also been used to observe the second-ordertransverse Doppler effectpredicted by the theory of relativity, because of very high energy resolution. More recently,
Mssbauer spectroscopy has been instrumental in developing an understanding of the structure
and function of iron containing enzymes and the model complexes synthesized to mimic thefunctions of these enzymes. Some examples of enzymes characterized in this way are:
ribonucleotide reductasemethane monooxygenase,tryptophan dioxygenase,[17]deoxypusine
hydroxylase,[18]protocatechuate 2,3 dioxygenase, andcytochrome ba3
Mossbauer spectroscopy has also been used very successfully to investigate the electronicstructure ofheterobimetallic complexes.[21][22][23][24]
Mssbauer spectrometers
http://en.wikipedia.org/wiki/Ligandhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-9http://en.wikipedia.org/wiki/Fischer%E2%80%93Tropsch_synthesishttp://en.wikipedia.org/wiki/Magnetitehttp://en.wikipedia.org/wiki/Cementitehttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-10http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-10http://en.wikipedia.org/wiki/Antimonyhttp://en.wikipedia.org/wiki/Olefinshttp://en.wikipedia.org/wiki/Calcinationhttp://en.wikipedia.org/wiki/Calcinationhttp://en.wikipedia.org/wiki/Tin_dioxidehttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-11http://en.wikipedia.org/wiki/Transverse_Doppler_effecthttp://en.wikipedia.org/wiki/Theory_of_relativityhttp://en.wikipedia.org/wiki/Theory_of_relativityhttp://en.wikipedia.org/wiki/Methane_monooxygenasehttp://en.wikipedia.org/wiki/Methane_monooxygenasehttp://en.wikipedia.org/wiki/Methane_monooxygenasehttp://en.wikipedia.org/w/index.php?title=Tryptophan_dioxygenase&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-17http://en.wikipedia.org/w/index.php?title=Deoxypusine_hydroxylase&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Deoxypusine_hydroxylase&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-18http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-18http://en.wikipedia.org/w/index.php?title=Protocatechuate_2,3_dioxygenase&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Protocatechuate_2,3_dioxygenase&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Cytochrome_ba3&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Cytochrome_ba3&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Heterobimetallic_complex&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Heterobimetallic_complex&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-21http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-22http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-23http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-24http://en.wikipedia.org/wiki/Ligandhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-9http://en.wikipedia.org/wiki/Fischer%E2%80%93Tropsch_synthesishttp://en.wikipedia.org/wiki/Magnetitehttp://en.wikipedia.org/wiki/Cementitehttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-10http://en.wikipedia.org/wiki/Antimonyhttp://en.wikipedia.org/wiki/Olefinshttp://en.wikipedia.org/wiki/Calcinationhttp://en.wikipedia.org/wiki/Tin_dioxidehttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-11http://en.wikipedia.org/wiki/Transverse_Doppler_effecthttp://en.wikipedia.org/wiki/Theory_of_relativityhttp://en.wikipedia.org/wiki/Methane_monooxygenasehttp://en.wikipedia.org/w/index.php?title=Tryptophan_dioxygenase&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-17http://en.wikipedia.org/w/index.php?title=Deoxypusine_hydroxylase&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Deoxypusine_hydroxylase&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-18http://en.wikipedia.org/w/index.php?title=Protocatechuate_2,3_dioxygenase&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Cytochrome_ba3&action=edit&redlink=1http://en.wikipedia.org/w/index.php?title=Heterobimetallic_complex&action=edit&redlink=1http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-21http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-22http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-23http://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-247/29/2019 Mossbauer spectra
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A schematic view of mssbauer spectrometer
A Mssbauer spectrometer is a device that performs Mssbauer spectroscopy, or a device that
uses the Mssbauer effect to determine the chemical environment of Mssbauer nuclei present in
the sample. It is formed by three main parts; a source that moves back and forth to generate adoppler effect, a collimatorthat filters out non-parallel gamma raysand a detector.
A miniature Mssbauer Spectrometer, named (MB) MIMOS II, was used by the two rovers in
NASA'sMars Exploration Rovermissions.[25]
Notes on 57Fe Mssbauer spectroscopy
Sodium nitroprusside is a common reference material
The Mssbauer parameters: chemical isomer shift and quadrupole splitting are generally
evaluated with respect to a reference material. For example, in iron compounds, the Mssbauer
parameters were evaluated using iron foil (thickness less than 40 micrometers). The centroid ofthe six lines spectrum from metallic iron foil is 0.1 mm/s (forCo/Rh source). All shifts in other
iron compounds are computed relative to this 0.10 mm/s (at room temperature), i.e., in this case
isomer shifts are relative to Co/Rh source. In other words, the centre point of the Mssbauer
spectrum is zero. The shift values may also be reported relative to 0.0 mm/s, here shifts arerelative to the iron foil.
To calculate outer line distance from six line iron spectrum:
http://en.wikipedia.org/wiki/Doppler_effecthttp://en.wikipedia.org/wiki/Collimatorhttp://en.wikipedia.org/wiki/Gamma_rayshttp://en.wikipedia.org/wiki/Gamma_rayshttp://en.wikipedia.org/wiki/MIMOS_IIhttp://en.wikipedia.org/wiki/NASAhttp://en.wikipedia.org/wiki/NASAhttp://en.wikipedia.org/wiki/Mars_Exploration_Roverhttp://en.wikipedia.org/wiki/Mars_Exploration_Roverhttp://en.wikipedia.org/wiki/Mars_Exploration_Roverhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-25http://en.wikipedia.org/wiki/Cobalthttp://en.wikipedia.org/wiki/Cobalthttp://en.wikipedia.org/wiki/Rhodiumhttp://en.wikipedia.org/wiki/File:Sodium_nitroprusside_M%C3%B6ssbauer_spectrum.svghttp://en.wikipedia.org/wiki/File:Sodium_nitroprusside_M%C3%B6ssbauer_spectrum.svghttp://en.wikipedia.org/wiki/File:Mossbauer_Spectrometer.jpghttp://en.wikipedia.org/wiki/File:Mossbauer_Spectrometer.jpghttp://en.wikipedia.org/wiki/Doppler_effecthttp://en.wikipedia.org/wiki/Collimatorhttp://en.wikipedia.org/wiki/Gamma_rayshttp://en.wikipedia.org/wiki/MIMOS_IIhttp://en.wikipedia.org/wiki/NASAhttp://en.wikipedia.org/wiki/Mars_Exploration_Roverhttp://en.wikipedia.org/wiki/M%C3%B6ssbauer_spectroscopy#cite_note-25http://en.wikipedia.org/wiki/Cobalthttp://en.wikipedia.org/wiki/Rhodium7/29/2019 Mossbauer spectra
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where c is the velocity of light in m/s, Hint is the internal magnetic field of the metallic iron(33 T), N is the nuclear magneton (3.152451232610
8 eV/T), E is the excitation energy
(14.412497 keV),gn is the ground state nuclear splitting factor (0.09062/(I), whereIsospinI= 12)and g*
n is the excited state splitting factor of57Fe (0.1549/(I), whereI= 32).
By substituting the above values one would get V= 10.62 mm/s.
Other values are sometimes used to reflect different qualities of iron foils. In all cases any
change in Vonly affects the quadrupole splitting and not the isomer shift. As the IBAME, the
authority for Mssbauer spectroscopy, does not specify a particular value, anything between10.60 mm/s to 10.67 mm/s can be used.
http://en.wikipedia.org/wiki/M/shttp://en.wikipedia.org/wiki/Tesla_(unit)http://en.wikipedia.org/wiki/Nuclear_magnetonhttp://en.wikipedia.org/wiki/Nuclear_magnetonhttp://en.wikipedia.org/wiki/Electronvolthttp://en.wikipedia.org/wiki/Isospinhttp://en.wikipedia.org/wiki/Isospinhttp://en.wikipedia.org/w/index.php?title=International_Board_on_the_Applications_of_the_M%C3%B6ssbauer_Effect&action=edit&redlink=1http://en.wikipedia.org/wiki/M/shttp://en.wikipedia.org/wiki/Tesla_(unit)http://en.wikipedia.org/wiki/Nuclear_magnetonhttp://en.wikipedia.org/wiki/Electronvolthttp://en.wikipedia.org/wiki/Isospinhttp://en.wikipedia.org/w/index.php?title=International_Board_on_the_Applications_of_the_M%C3%B6ssbauer_Effect&action=edit&redlink=1