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    Radiation ProcessingBasic Aspects

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    , , ,

    Radiation Chemistry: Developments Discovery of X-rays, Roentgen 1895 Discovery of Radioactivity, Becquerel 1896 Since the fifties, our understanding of radiation physics,chemistry and biology has increased tremendously

    aca~ 1200-a- 10008. 800o 600c::.2 400..-ca 200( ):E 0 ' " r , , ,i 1 9 ~ 1 ~ 0 1 ~ 0 1 ~ 0 1 9 6 0 1 m 1 9 0 0Year

    Swallow (1960) and Helman and Ross (1980)

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    Radioactivity Consists of , ~ and "I - emissions with energiescharacteristic of the emitting nucleus

    a- particles: Helium nucleus, He2+ ion, emitted from the nucleusp- particles: Fast electrons emitted from the nucleus1- rays: Uncharged electromagnetic radiation emittedfrom the nucleus, usually along with p-particle

    ~ r b i t a l electrons

    An Atom

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    Different Penetration ofVacuumUV, a, pand 'Y...(I )3:oc..enc.-..co......(I )c(I )c..1 UV

    ConcreteAluminum ~ = ~ ~ ~ = = ~Paper

    The difference in penetration is a result of differentprobabilities of interaction of a., B, 'Y and vac-Uvradiation with orbital electrons ot a molecule

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    Induced Radioactivity Induced radioactivity ~ r o d u c e d by nuclearreactions of H+, D+, He +, neutrons andy-rays

    27Al + 4He2+ (a) - - - . . 30p + n30p e+ + 30Si

    Neutrons are the most important initiatorsof induced radioactivity

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    Neutron-InducedRadioactivityn + 2H (3H) 3He + e- (1 112 -12.4y)n + 27Al ~ (28AI) 28Si + e- (1 112 - 2.3min)n + 113Cd (114Cd) 114Cd + 'Y

    (1 112 - 43d)

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    Some Threshold Values for NuclearActivation2H + "I (2.23 MeV)-..... 1H + n

    181T a + "I (7 .64MeV) 180Ta + n197Au + "I (8.07 MeV) 196Au + n204Pb + "I (8.38 MeV) 203Pb + n70Zn + "I (9.29 MeV) 69Zn + n65CU + "I (9 .91MeV) 64CU + n(IAEA Technical Report No. 188, 1979)

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    Induced Radioactivity The energy levels permitted for use in foodirradiation are specifically selected to avoid anyconditions which could induce significant leversof radioactivity in the treated commodities

    The permitted energy levels are:X-rays (or "I -rays) ~ 5 MeVElectrons ~ 10 MeV For radiation processing of items other than food,electrons or X-rays up to 10 MeV can be used asneeded, without concerns about inducedradioactivity

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    Induced Radioactivity vsElectron Energy

    maximum50 allowedenfrgyo ........... . . . . , . . ~ - - - .....--....9 11 13 15

    300250

    -

    ~...-->---u ~co--o c: 200-- ~-g ~ 150a: co~"=:: 100Q).c( , ) ~~ c o,,-c:

    Electron EnergyJMeV)- - - - - '

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    Natural and Induced Radioactivity fromVarious Sources (Becker, 1979)

    -Natural activity in average human body-Natural activity/kg meat-Allowed activity of 1311per litre of milk

    -Increase in activity from fallout/kg meat-Reported increase in activity in milk atTflree Mile Island16 MeV

    14 M e V 1 ; : : = - - - - . . . . ~

    lOS104UP1()2101110-110-210-310-4 12 MeV -1 Disintegeration/day10-5 10 MeV1-------\ -1 Disintegration/year10-6.1.::==:======::::1

    oenco.--C )(I )-.-o.-C(, ).-Eo-

    - In "pure" organic polymers, induced radioactivity shouldbe lower than in foods; in metals it would be higher

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    Sources for Radiation Processing Natural radioactive isotopes are not suitable forradiation processing Radiation processing feasible with artificiallyproduced radioactive isotopes

    60CO (1), 137CS (1) Radiation processing helped by the development ofelectron accelerators to produce

    Electron (e-) beams, X-raysMetal

    e- ( : ~ 1 0 M e V ) - - - - ~ .. X-rays In electron accelerators one can choose the electronenergy, as required for a given application The mode of action of 'Y- and X-rays is exactly the same The mode of action of e- from accelerators and~ particles from radioactive isotopes, is also the same

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    Radioactive Decay of the Gamma-Emitting Isotopes

    1, 0.662MeV(83% ) ; e",K{90/0),L (2% )

    ~ __137Ba

    Stable 137Ba

    137Cs(Half-life 30.2 y)P,0.514MeV(mean 0.175),

    94.6%

    p, 1.176 Me{mean 0.42MeV),5.4%, 1.333MeV,100%Stable 60Ni

    6oCo-ttlalf-life 5.27 y)p, 0.313 MeV(mean 0.094MeV),99.8%~ - - 6 o N i

    B,1.486 M W 'Y, 1.173 MeV(mean 0.62 (99.8%)MeV), 0.2% - __ 6oNi

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    I Radioactive Decay of 137Cs and 60Co I10090- 80 137CS:::Re.... 70

    >- 60....- 50>.- 40..(, ) 30 60CO

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    Interaction of Ionizing Radiationwith MatterA Simplified Picture

    The energy transfer mechanism involvesinteractions between the incident particlesor photons and orbital electrons of theatomic/molecular constituents of a substrate

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    Interaction of Ionizing RadiationWith Mattera, por ~ Orbital electron ejectedas secondary electron

    - - v . ~ - - - - " " : : : : : : " : T h e incident particleor photon (withreduced energy)

    Energy Deposition Event(for details see Klots in Ausloos, 1968) The probability of interaction follows the order, a.> ~ >"{and hence the order of their penetration in matter Energy loss per event, mainly 20100 eV Radiolysis similar to vacuum UV photolysis

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    Energy Deposition

    Ia Particles I.IFast ElectronsI. . ... .

    .. .. .. . ,.. .. .. '.."'... . _ , .... e ..... .", r . . . .

    ...._1.:....

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    A Typical Spur in Water

    2.3 nm

    G(e-aq) - 5G(.OH) - 6

    [e-aq ] ~ . O H ] ~ 0.1 mol.dm-3 (Av)a[ .OH ] ~ 2 mol.dm-3 (Spur Core)b

    Adapted from Singh and Singh, 1982. Initial concentration,(a) averaged over total spur volume (diameter 4.6 nm); (b)within the spur core (diameter 1.5 nm)

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    Distribution of Ions and Excited Moleculesin the Track of a Fast Electron

    ISpurs 5000 eVThe quantity of energy deposited determines whether an individualevent will give rise to a spur or a larger group of ions and excited

    molecules Blobs (100-500 eV) and short tracks 5000 eV) can be considered asgroups of overlapping spurs Delta rays are secondary electrons of energy less than 10,000 eVFor 10 MeV e-: 75% spurs, 17% short and branched tracks, 8% blobs(Spinks and Woods, 1990)

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    Basic Similarity of Radiolytic Effects by DifferentHigh Energy Radiations

    Substratet

    Secondary Electrons withSuccessivelyLower Energies (eV)

    Ener9.YDeposition -a .e- or R I-_Mev Substrate Ions + ExcitedP 1\1\1"1

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    Energy Absorption in Mixtures Components of a mixture absorb energy in proportionto their respective electron densities

    Electron density=number of orbital electronsper unit weight

    For gamma and electron irradiation of organicaqueous systems, a reasonable approximation is thatthe components of a mixture absorb energy inproportion to their weightBiological System, 75% water and 250/0 organicEnergy absorbed, ""75% by water and

    ",,25% by organic

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    Radiation ProcessingPhysical Effects

    Widely Used in Welding Industrial Radiography Ion Implantation Gemstone IrradiationSee Woods and Pikaev (1994), for details andret"erences

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    Radiation ProcessingChemical Effects

    1. Background2. Basic Aspects3. Formation and Reactions of Short-LivedReactive Species4. Products From Typical OrganicCompounds

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    Irradiation, Overall EffectSubstrate f I I ( - ~ Ions, Excited States,Free Radicals

    ~Products

    Generally, higher the yields of excited states, the lowerthe overall decomposition, e.g., aromatic compoundsdegrade less than aliphatic compounds

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    - + - Bond BreakageBegins

    Forms ofEnergy Supply(1) Heat(Pyrolysis)

    Temperature=== I P Excitation leveldependent on theenergy of the quanta(2) Light(Photolysis) Energy__Le v e r s - _ 8281hV Temperature of theG r o u n d - - 80 system generallyunchanged

    Bond breakage generally from 81 or higher levels (dependenton energy of quanta and bond dissociation energies)

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    High Energy Radiation(Radiolysis)

    IP --- Ionization and excitation Singlet and triplet states Variety of bonds broken

    T2 Bond dissociation energy-- still important__T1 Ionic reactions alsoimportant

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    Singlet and Triplet Energy Levels ofDonors and Acceptors

    I-

    -,

    An!bracen:.-Biacetyl

    -,

    N ~ h t h a l e n e

    I-

    ,

    --,

    I-

    I-

    8.-----------------.----...."~ - - H e x a n e ClTriplet7 +--I I - - - - - - - - - - , ~.....------.B'ut,--en-e------I CISinglet:> 6 +------ l..!- 5 +--I Benzene~ 4+--1...Q) 3 +--Ic: 2W +--I1 +--Io -- The singlet energy levels of c-hexane and 2butene areestimates (Ausloos, 1968) Singlet state transfers energy to lower singlet state andtriplet state only to lower triplet state

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    Water is the most studied l iquid in radiation chemistry

    Radiolysis ofWater

    The species present at 10-7s :e-aq ,H, OH, H20 2' H30 + ,02-

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    Transition From I n h o m o ~ e n e o u s to H o m Q g ~ n e o u sDistribution ofFree Raaicals in Liquid Water( i ) 'y- Irrad_10-125

    o

    o

    o

    ( i i ) G (e-aq)-2.7G (.OH)-2.7

    HomogeneousDistribution(.CH, e-aq' .H)[e-aq ] ~ [ . O H ] ~ 10-9 mol.dm-3('Y)c

    ~ 10-3 t010-6 mol.dm-3 (e-)d( i ii) 0 0 o ~ 00 0 0 0 g ~ 0 0 [Spur] -Very high number

    (T 0 0 008 3 ao ~ o 0 ~ o 000 [ e - a q ] ~ [ . O H F O . 1 mol.dm- (Av)0 0 0 0 0 0 0o 0 0 ~ 0 0 0 0 c [.OH] ~ 2 mol.dm-3 (Spur Core)ba. Averaged over total spur volume; b. Initial Concentration withinthe spur core; c. 'Y - Irradiation; d. e-- Irradiation

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    Transition From Inhomogeneous toHomogeneous Distribution ofFree Radicalsin Liquid Water

    (i) Represents spur formation on energy absorptionfrom a single gamma photon in 10-12 s or less

    (ii) Shows homogeneous distribution of reactivespecies on diffusion of spurs in about 10-7 s(iii) Represents spur formation on energy absorptionfrom a single electron in 10-12 s or less. The higher

    spur concentration [spur] on electron irradiation isnot drawn to scaleSingh (1991)

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    pH Dependence ofYields on RadiolysisofWater

    ~ 3=- 2I~ 1

    O ~ ; ; ; ; ; ; : : " - - J I : 4 - , . - __ - __ - ~ ~ : ; ; . J1

    The pH range of most foods lies between 2 and 8

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    Products

    Radiolysis ofOrganic LiquidsEVENT

    I< 10"1f,l--,/"RH "'-.t 10-14S IRH* RH+ + e-.----------..I ,., 10-11 5V < 10-125 Solvation(RH dependent)R + H I""10-105 I -(eS01v )

    1"--""1-0-1-05 1\Products

    Excitation longer lived and more important in organicsystems, than In water Ionic species formed but much shorter lived than in water In the presence of air/02, peroxy radicals and 2-" formed

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    Products

    RADIOLYSIS OF ORGANIC LIQUIDSEVENTRH< 10-14S I ' I ' ~ "'-..., < 1014S/"" .,.,

    / 'RH* RH+ + e-,., 10-11S/ \ < 10-12S Solvation\ (RH dependent)R + +I ""1 0-1Os -(esolv )

    ""10-10s \Products

    Excit!ltion longer lived and more important in organic systems,than In water Ionic species formed but much shorter lived than in water In the presence of air/02, peroxy radicals and 02- formed

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    Basis for Beneficial Effect of Irradiationo

    r::::o.--.)~~-J)Q)c'#. Background per annum100 --p.loI. . . . . . . . .- . . . . . .- . . , . . -. . . . . . . . . . . . . .- . . , . . . ; - - ....... . . " . . .....-ol10-1 10 0 101 10 2 10 3 10 4 10 5 10 6 10 7 10 8

    Dose (Gy) These differential senstivities of different functionalentities to inactivation are the basis of beneficialeffects of irradiation

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    IrradiationMicroorganism Inactivation

    Irradiation used to control microorganismlevels (food, sewage, medical devices)

    Irradiation harmful to humans; so, exposureof humans kept within safe limits

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    Radiation-Inactivation ofE. coli1c:0 10-1.--ct1 10-2..U.

    C ) 10-3c:.->.- 10-4>..::::JCJ) 10-50 0.4 0.8 1.2

    X-Ray (kGy)E.coli cultured aerobically in broth and irradiated in02-saturated or N2-saturated buffer (Casarett,1968)

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    Concluding Remarks Physicists, chemists and biologists havecontributed to the high level of understandin9of the basic aspects of radiation science, whichforms the foundation of radiation processing One of the biggest industrial applications ofradiation processing, crosslinking ofpolyethylene and the heat-shrink phenomenon,were discovered by Prof. Arthur Charlesby in1957 when he was investigating the effects ofhigh energy radiation on polymers