Radioisotope Techniques

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    Radioisotope Techniques

    Mak Oi Tong

    Department of Life SciencesNational Cheng Kung University

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    Radioisotope

    n Atoms with unstable nuclei transform

    into other stable atoms.

    n Results : Release of energetic particles

    or radiant energy,

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    Atoms, isotopes and radioisotopes

    n Atomic number, mass (mass number or atomic weight)

    n Carbon : 12C6n atomic number = 6 and atomic mass = 12

    n Contains 6 protons, 6 neutrons and 6 electrons.

    n Isotopes : atoms have identical chemical properties butdifferent atomic weight.

    n e.g. 11C, 12C, 13C and 14C

    n14C6 >

    + 14N7 +e- (antineutrino)

    n11C6 >

    + + 11B5 +e (neutrino)

    n Ratio of neutrons and protons

    n Lighter atoms 1:1 and 1.5:1 at high atomic number

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    Types of radioactive decay

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    Negative-Beta (electron) emission

    n Ejected electrons emit from the nucleus

    which are identical with the orbital electron in

    mass and charge (neutron to proton).n

    3H1 >3He2 +

    +e- (antineutrino)

    n14C6 >

    14N7 + +e- (antineutrino)

    n

    32

    P15 >32

    S16 +

    +e- (antineutrino)n

    35S16 >35Cl17 +

    +e- (antineutrino)

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    Positive-Beta (positron,+) emission

    n + is same mass as electron but having opposite

    charge, and it will emit as gamma (

    ) radiation.n + + e- > (1.02 MeV)

    n11C6 >

    11B5 ++ +e (neutrino)

    n13N7 >

    13C6 ++ +e (neutrino)

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    Decay by electron capture

    n Conversion of a nuclear proton into a neutron

    by capture one of the two electrons in theinnermost K-shell, ie. K-capture (KC) and

    emission of a positron+.

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    Decay by-radiation

    n -Ray emission occurs after or+

    emission.

    D b i l i i

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    Decay by- particle emission

    n Heavy atoms with more than 82 protons will

    emit an-particle which is a helium nucleus

    of atomic mass number of 4 (2 protons and 2

    neutrons) with a charge of +2.

    n226Ra88,

    235U92 etc. are examples for-

    particle emitters and are not for biochemical

    studies but for radiological toxicity.

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    radioactive isotopes

    n Pierre and Marie Curie introduced the term

    radioactivity to designate the process of spontaneousemission of radioisotope.

    n Artificial production of radioisotopes is normallydone by neutron bombardment.

    n Other methods: -particle, proton and deuterons

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    n To-day, over 1500 isotopes are producedartificial produced.

    n On earth, radioisotopes are produced byneutral bombardment, and 14C and 3H(tritium) are in equilibrium.

    n Radioisotopes can be used for radiocarbon(14C) dating.

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    Properties of radioactive emissions

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    Energy of-particle emissions

    n -

    ,+

    and e-

    travel near the speed of light, 3x 1010 cm/s or 3 x 108 m/s.

    n Emax is the maximum energy value, and the

    Eave Average) is equal to 1/3 of Emax.

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    Interaction of particular with their

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    Interaction of -particular with their

    environment

    n - will cause electron excitation and emit UV or

    visible light.n In air, about 34 ev is required to produce one ion

    pair.

    n An ejected electron, with an energy of 1.5 MeV,will travel about 2 meters in air, and about 1 cm intissue.

    n Eventually the ejected electron will be captured by

    an empty electron orbit of a positive ion.n When a positron encounters an its electron, the two

    particles annihilate (combine) each other and theirmasses are converted into electromagnetic-

    radiation which is I the form of two 0.51-Mev

    amma ra at on an ts nteract on

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    amma ra at on an ts nteract onwith matter

    n Gamma rays are high energy photons or light

    particles that are electrically neutral with zero massand consequently can penetrate matter readily.

    n -Ray is emitted from the nucleus with discreteenergy range between 10 KeV to 3 MeV.

    n Many isotopes emit of- ray of several energies indiscrete steps (Fig. 6.2).

    n Photoelectric effect is a- ray of relatively low

    energy (

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    n The Compton effect results when- rays of

    medium energy (>0.1 MeV) undergo elastic

    collisions with loosely bound orbital electron and aportion of the- ray energy is transferred to the

    ejected electron.

    n

    The photon is deflected in a new direction withreduced energy and undergo several more similar

    collisions before losing all its energy.

    n Compton electrons have a wide range of energies

    and these electrons will produce secondaryionization as they travel through the medium,

    dissipating their energy.

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    n Pair production results when a relativelyenergetic (>1.02 MeV)- ray interacts with

    a nuclear force field.n The photon has all its energy converted into a

    positron and an electron.

    n This is essentially the conversion of energyinto mass.

    n Both the ejected positron and electron may

    cause ionization of atoms in their paths, andcollies together.

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    Kinetics of radioactive decay

    n The process of decay of a radioactive nucleus into a

    stable, nonradioactive nucleus is irreversible.

    n Rate of decay (particle emission) is equal to the rate

    of disintegraton of the nuclei, which is proportional

    to the number of radioactive nuclei present.

    n Rate of decay decreases exponentially with time.

    n It is independent of pressure, temperature and other

    chemical and physical changes.n The rate is first order reaction.

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    n Rate of decay:

    n N = amount of radioactive nuclei present

    n = decay constant

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    n Activity is the quantitative measurement of

    radioactive and if the activity of sample is A

    (by detector), it becomes the counting rate ofthe sample.

    Efficient of detector

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    Half-life (t )

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    Units used in radioactive measurements

    n The electron volt

    n One electron volt (1 eV) is the kinetic energydeveloped by an electron when it is acceleratedthrough a potential difference of 1 volt in a

    vacuum.n 1 eV is equal to 3.85 x 10-20 calories or 1.602 x

    10-19joule.

    n It is normally expressed in KeV or MeV.

    n The electron emitted from 14C has an averageenergy of 4500 eV per nucleus (atom).

    Th i h i f di i di i i

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    n The curie: the unit of radioactive disintegration

    n One curie is equal to the number of disintegration per

    second in 1 gram of pure radium 226.

    n It is also equal to 2.22 x 1012 disintegration per minute

    (dpm).

    n One becquerel (one disintegration per second) is equal to

    3.70 x 1010 becquerels.

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    Safety in handling radioisotopes

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    Safety in handling radioisotopes

    n First to know whether it is- or+ -ray isotopes.

    n Prevent injection, inhalation or absorption ofradioisotopes in human body.

    n Laboratory coat, plastic gloves etc. Should be worn for

    body protection.n Restricted areas for handling radioisotopes must be

    labeled, clean and neat.

    n Covered with plastic absorbent paper with a tray line.

    n Have special containers for any radioisotope disposal

    such as glasses, plastic, paper, water and organic

    solvent.

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    n Monitor the working place routinely for any

    contamination of radioactivity by using Geiger-

    Muler survey monitor for strong and ray.

    n Wear a personal dosimeter for high energy

    radioisotopes.

    n Wash immediately if any contamination is present.n If skin has contacted with radioisotope, wash with

    immediately for at least 2 minutes.

    n Special care is required for anyone handling 125I or131I because of the effects on thyroid gland in

    human body.

    Statistics of counting radioisotopes

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    Statistics of counting radioisotopes

    n Compare Fig. 6.1 and Fig. 6.5.

    n Standard deviation s:

    n A more common situation is:

    n Confidence of the true value.

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    P l i d d d i i (% RSD)

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    n Percent relative standard deviation (% RSD)

    n For sample comparison, % RSD is generally

    required.

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    Measurement of radioactivity

    n By gas ionization.

    n By scintillation counting

    By gas ionization

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    By gas ionization

    n When a energetically charged particle, such

    as- particle, passes through a gas, itselectrostatic field displaces orbital electron

    fro the gas molecules close to its path.

    n This displacement produce a positive ionfrom the other part of the molecule, resulting

    an electron pair.

    By gas ionization

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    y ga a

    n If an electric field is applied in the chamber,

    the displaced electrons are accelerated towardthe anode and the positive ions move towardcathode slowly (because of their larger mass).

    n

    If higher electric fields are applied, theelectron displaced by the first- particlecollision is accelerated and collides with othergas molecules to produce additional ion pairs.

    n This result is an amplification of the numberof electrons from the first electron, giving ashower of electrons.

    monitor

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    n A type of radioactive detector.

    n It is a gas-filled tube with cylindrical cathode

    and a fine wire anode.

    n A common gas mixture is the so called Q-gas

    which is 1.3 % isobutane in helium.

    n One end of the tube has a window through

    which the- particles from the radioactive

    sample.

    monitor

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    n A voltage potential is applied between the electrodes

    of the tube and produces shower

    n The electrons are collected at the anode within amicrosecond, and a strong electrical pulse is formed.

    n The number of electrons collected is proportional to

    the number of initial ionization, and is proportionalto the number of- particles entering the chamber.

    n The region is called proportional region.

    n

    Efficient, for

    14

    C about 1 to 5 % and for

    3

    H is nearlyzero.

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    By scintillation counting

    n Use scintillator or fluors for- and- ray counting.

    n Scintillator can absorb radiant energy to form excited atoms

    or molecules and return rapidly to ground state, releasing

    excitation energy, to form photon and heat.

    n Amount of photon released directly related to the amount of

    radiant energy.

    n

    Liquid scintillation counting is that the scintillators aredissolved in a solvent called cocktail.

    By scintillation counting

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    y g

    n Steps for photon formation:

    n - Radiant energy is absorbed by solvent and become excited.

    n The solvent transfers the the excited energy to the scintillator to

    cause excitation.

    n The scintillators release photon which is detected by the phototubes.

    n The phototube converts photons into amplified numbers of electron,and then becomes voltage pulse by a pulse height analyzer, and this

    is called- and- scintillation counter.

    n - energy spectrum refers to Fig. 6.12.

    n

    Dual-labeled mixture activity determination refers to Fig.6.13.

    Cocktail composition and samplepreparation

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    preparationn Primary fluor is 2,5-diphenyloxazole (PPO).

    n Secondary fluor is 1,4-bis-2-(5-phenyloxazolyl) benzene(POPOP).

    n Common solvents: toluene and dioxanen Toluene is used for organic compounds.

    n

    Dioxane is used for aqueous samples.n Heterogeneous counting is that the radioactive samples are

    in solid support.

    n Homogeneous counting is that the radioactive samples arein dissolved form.

    n Background counting is caused by electronic noise, cosmicradiation and other natural radioisotopes present.

    n Cerenkov counting is used for direct- particle countingwithout fluor, only for high energy- emittor, e.g. 32P.

    Quenching

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    n It is the process that causes a reduction in the amount of

    fluorescence produced by

    - emission in a liquidscintillation cocktail, reduction amount of light reaching the

    photomultipler tube.

    n Chemical quenching is that the transfer of energy is

    interfered from solvent to fluor molecules (fluorescencereduction).

    n By acid

    n By dipole-dipole interaction of quenching agent

    n Electron capture by quenching agent.

    n Color quenching is the presence of colored compounds

    which can absorb the photons emitted by the fluor, e.g.

    Pigment, blood.

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    Quench correctionn

    Internal standard method:n Add another non quenching radioactive standard and

    recounted.

    n External standard method:

    n Use of a highly radioactive- radiation source, e.g.226Ra or 137Cs, which is brought near to the test

    sample vial and the sample is recounted in a short

    time.

    n Efficient by ES refers to 6-19.

    S lid i till ti ti f di ti

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    Solid scintillation counting of radiation

    n

    A crystalline inorganic fluor, sodium iodide (NaI), withsmall amount of thallium (Tl) as activator.

    n - Rays interact with crystalline fluor to form ion pair, the

    Compton effect and induce photoelectric and excite

    crystalline fluor, finally produce photon to reachphotomultiplier tube.

    n The crystalline fluor is sealed in a metal cylinder from

    external light.

    n The cylinder must be hermetically sealed because ofhygroscopic of NaI.

    n It is designed for the counting of125I, 51Cr and 60Co.

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    A toradiograph

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    Autoradiography

    n A technique for the determination the location of

    radioisotopes in tissue, tissue sections, chromatograms and

    gels.

    n It is a non-destructive method for radioactive compounds,

    and can be isolated and recounted.

    n Results are shown on a X-ray film and developed.

    n The- ray hits the silver bromide of the film and reducing

    to metallic silver from silver ions, and black spots will be

    appeared.n For best darkening of the film, at least 1 x 106 (- particle)

    passing through the film per cm2 per minute.

    A di h

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    Autoradiography

    n If sample contains 1 x 103 cpm/cm2, it will take about 100

    minutes or 17 hours to induce the black spot.

    n For weak ray, enhancer ( fluorography, PPO) is need to

    enhance the sensitivity, particularly 3H.

    n The photoelectric effect are more stable under -50 to -80C

    about 4x more stable.

    n The resolution can be increased by decreasing the thicknes

    of the sample and the distance between sample and the fil

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    M h d f l b li bi h i l

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    Methods of labeling biochemicalcompounds

    n Two general methods:

    n biosynthesis and

    n chemical synthesis.

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    Biosynthesis

    n Used by either whole organisms (cells) or specific enzymesto synthesize radioactive compounds.

    n The common used radioisotopes are 14C, 32P and 35S.

    n Factors for the successful use of biosynthesis:

    n By using whole organism, labeled compound(s) must beaccumulated in large number from starting compound.

    n For using a specific enzyme, the enzyme must be easily isolatedand the substrate is readily available, and the labeled compoundmust be isolated and purified from the reaction mixtures.

    n

    For using microorganism, labeled compound is isolated from themicroorganism or the cell-free culture supernatant fluid.

    n Whole organism biosynthesis gives a relatively largenumber of labeled products but enzyme synthesis gives onlyone or specific labeled products.

    Ch i l h i

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    Chemical synthesisn

    Products can be labeled in one or few positions.n Starting materials always be scarce and expensive.

    n Results give low yield.

    n Give a racemic mixture of optical isomers, e.g. D- and L-

    isomers of amino acids.n Types of labeling of compounds:

    n Labeling of proteins.

    n Labeling of nucleic acids.

    n Formation of14C carbon-carbon bonds.

    n Synthesis of tritium labeling [3H] compounds from NaB3H4.

    n Synthesis of35S-labeled L-cysteine

    T f di h i l l b li

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    Types of radiochemical labelingn

    Isotopically: one or more radioactive atoms have replacedstable atoms of the same element, e.g.

    n3H1

    1H1,14C6

    12C6,35S15

    31P15

    n They are the same molecules.

    n

    Nonisotopically: a radioactive isotopes has beensubstituted for a stable atom of another element, e.g.

    n125I for 1H1

    n Three forms of labeling positions:

    n

    Specific: [1-14

    C]-D-glucosen random: randomly distributed (G-).

    n *CH3-CH2COOH, or CH3-*CH2COOH or CH3-CH2*COOH

    n Uniform: all related atoms are labeled, [U-], e.g. [U-14C]-

    sucrose.

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    Radioimmunoassayn Ab (antibody) + Ag (antigen) Ab-Ag complex

    n Present an abstract about the basic principle and

    application of radioimmunoassay.

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    Designing a radioisotope experiment

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    Designing a radioisotope experiment

    n

    First and foremost in the design of anyexperiment is the formulation of the question tobe studied, the purpose and nature of theexperiment.

    n Next is what experimental techniques toanswering the question.

    n Is radioisotope necessary ? What type ofradioisotope ?

    n

    Which position and and which type of labeledcompound.

    n Availability of the labeled compound.

    n How much specific activity and amount of

    radioactivity required

    Designing a radioisotope experiment

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    Designing a radioisotope experiment

    n What is the cost of the labeled compound ?n Experimental methods.

    n What type of detection system and its efficiency ?

    n The dilution effects and the yield of theradioisotope.

    n Control and correction factors needed.

    n

    Expression and interpretation of the results, andfinally

    n The possible isotope effects and possible effects

    of radiation damage.