Radiation Effects of a Nuclear Bomb - University of Notre...

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Radiation Effects of a Nuclear Bomb Beside shock, blast, and heat a nuclear bomb generates high intensity flux of radiation in form of γ-rays, x-rays, and neutrons as well as large abundances of short and long-lived radioactive nuclei which contaminate the entire area of the explosion and is distributed by atmospheric winds worldwide. T 1/2 =5730y Effective half- life ~5-10 y (photosynthesis)

Transcript of Radiation Effects of a Nuclear Bomb - University of Notre...

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Radiation Effects of a Nuclear BombBeside shock, blast, and heat a nuclear bomb generates high intensity flux of radiation in form of γ-rays, x-rays, and

neutrons as well as large abundances of short and long-lived radioactive nuclei which contaminate the entire area of the

explosion and is distributed by atmospheric winds worldwide.

T1/2=5730y

Effective half-life ~5-10 y(photosynthesis)

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14C distribution

+ nuclear test related 14C production

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Nuclear Bomb related Radiation Production

The units rad (rem) are a measure of radiation exposure!

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Monitoring radiation intensity

[ ]

⋅==

sdecays

dtdNCi 10107.31Classical Unit: 1 Curie [Ci]

[ ]

==s

decaydtdNBq 11Modern Unit: 1 Becquerel [Bq]

The so-called dosimetry units (rad, rem) determine the amount of damage radioactive radiation can do to the human body. They depend on the kind and nature of the incident radiation

(X-rays, γ-rays, α-particles, β-particle, or neutrons).It also depends on the energy loss of the particular radiation and the associated ionisation effects in the human body material.

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Radiation Detection

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Radiation Exposure & Dosimetry

Dose: DEm

=Amount of energy E deposited by radiation into body part of mass m. unit Rad or Gray

Equivalent Dose: H Q D= ⋅ Radiation independent doseQ is normalization factorwhich accesses the individual body damage done by the particular kind of radiationUnit Rem or Sievert

Photons: Q=1Neutrons: E<10keV Q=5Neutrons: E>10keV Q=15Protons: Q=5Alphas : Q=20

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UNITS OF RADIATION MEASUREMENTDosage units:The Sievert (Gray) is a measure of biological effect.1 Gray (Gy) = 1 Joule/kg (Energy/mass)1 Sievert (Sv) = Gray x Q, where Q is a "quality factor" based on the type of particle.

Q for electrons, positrons, and x-rays = 1 Q = 3 to 10 for neutrons, protonsdependent upon the energy transferred by these heavier particles. Q = 20 for alpha particles and fission fragments.

Converting older units: 1 rad = 1 centigray = 10 milligrays ( 1 rad = 1cGy = 10 mGy ) 1 rem = 1 centisievert = 10 millisieverts ( 1 rem = 1cSv = 10 mSv )

Nominal background radiation absorbed dose of 100 mrad/year = 1 mGy/yr. Nominal background radiation dose biological equivalent of 100 mrem/year = 1mSv/yr. Occupational whole body limit is 5 rem/yr = 50 mSv/yr. 2.5 mrem/hr or 25 uSv/hr is maximum average working level in industry.

Exposure rate from Naturally Occurring Radioactive Material; an empirically derivedconversion factor for Ra-226 decay series: 1.82 microR/ hour = 1 picoCurie/gram.

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Exposure to Natural and Man-made Radioactivity

Tobacco contains α-emitter 210Po with T1/2=138.4 days. Through absorption in the bronchial system smoking adds 280 mrem/year to the annual dose of US population

Total average annual dose:H ≈ 250-300 mrem

Average annual dose from nuclearbomb test fallout Hfo ≈ 0.06 mrem.

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Sources of Natural and Radioactivity

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Spectrum of CR

Cosmic Rays origin from:• solar flares;• distant supernovae;

Cosmic Ray Bombardment

Low energy CR

High energy CR

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Cosmic Rays in High AltitudeEarth is relatively protected from cosmic rays through atmosphere shield; typical exposure is H=3.2 mrem/h. Mountain climbers and airline crews and passengers are exposed to higher doses of radiation. Dose doubles every 1500 m in height. At 10 km height dose is about 100 times sea-level dose H=0.32mrem/h.

Example: Total dose H:• after 10h of flight:H=3.2 mrem,

• for round trip:H=6.4 mrem

• Frequent flyer with about 10 transatlantic flights/yearH=64 mrem/year.

Compare to natural dose (~200 mrem/y) !

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Observable Effects!

Husband’s ringwith transatlantichigh altitude dose

8 times more dose

Wife’s ringwith groundlevel dose!

Au γ-activity

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Natural Radioactivity in the US

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Long lived 40K Radioactivity40K has a half-life of T1/2=1.28·109 yearsits natural abundance is 0.021 % 40K

40Ar 40Ca

β+ β-

γ

40Ar40K

Potassium decay to Argon

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Internal γ GlowingOn average, 0.27% of the mass of the human body is potassium K of which 0.021% is radioactive 40K

with a half-life of T1/2=1.25·109 [y]. Each decay releases an average of Eavg= 0.5 MeV β- and γ-radiation,

which is mostly absorbed by the body but a small fraction escapes the body.

Calculate, how many radioactive 40K atoms are in your body system!

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Some Mass and Number Considerations

[ ] [ ]

[ ]

[ ]particlesNkg

mN

gparticlesmN

Nparticlesm

gmm

atomsKg

m.m.m

m.m

m

K

bodyK

body

K

Kbody

bodyK

bodyKK

bodyK

body

20

15

7237

2340

740

1083.6 :body 80for

gramm.in massbody theneedyou , calculate to

/1054.8

401067.510023.6

1067.5

10023.6of 40

10675000210 :body in theK e radioactiv of mass

00270 :body in theK potassium of mass

:body theof mass

40

40

40

4040

40

⋅=

⋅=

=⋅⋅⋅⋅

≡⋅⋅=

⋅≡

⋅⋅=⋅=∗

⋅=∗

−−

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Example: 40KCalculate the absorbed body dose over an average human

lifetime of t = 70 y for this source of internal exposure.

[ ]

∗ = = ⋅ ⋅

∗ = ⋅ = ⋅

= ⋅⋅

⋅ ⋅ ⋅ ⋅

= ⋅ = ⋅ = ⋅

= ⋅

− −

Dose DEm

t A KEm

Activity A K N T N

D y g mMeV

m

D MeV kg J kg Gy

with eV J

absorbed

body

avg

body

K K

bodybody

: ( )

: ( ) ln

[ ]ln

( . [ ] ). [ ]

. . [ / ] . [ ]

: [ ] . [ ]

40

401 2

15 1

10 2 2

19

40 402

702

4 88 1005

9 47 10 15 10 15 10

1 1602 10

λ

1.25 10 [y]9 (8.54

[ ] [ ] [ ]

[ ] [ ]JeVwith

GykgJkgMeVD

19

2211

10602.11:

1063.2/1063.2/1066.1

−−

⋅=

⋅=⋅=⋅=

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Prompt Release of RadiationNuclear bomb causes sudden release of a high flux on:

γ-rays E=hν≈1-10 MeV electromagnetic wavesx-rays E=hν≈1-100 keV electromagnetic wavesα-radiation 4He nucleiβ-radiation electrons and positronsneutrons neutronsheavy radioactive species (cause for delayed radiation)

The prompt radiation is absorbed in the surrounding Atmosphere according to exponential absorption law

I0 is the initial intensity and µ is the attenuation coefficient determined by the interaction probability of radiation with molecules and atoms in air.

deIdI ⋅−⋅= µ0)(

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Absorption probabilityAttenuation coefficient µ depends on energy and natureof particle, medium and interaction probability. High Coulomb scattering probability for charged particles, causes high absorption probability, results in short range!

1 m Concrete1 m Concrete

AlphaAlphaBetaBeta

GammaGammaNeutronNeutron

Energy Range(α) Range(β)keV cm cm

10 0.01 0.2100 0.10 16.0

1000 0.50 330.010000 10.50 4100.0

Main component gammas & neutrons

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Neutrons originatedsecondary γ radiation by inelastic neutronscattering as well as by neutron captureon nitrogen isotopesin the surrounding air.Secondary γ-productionenhances radiation fluxand radiation extension.

Spread of prompt & secondary γ-radiation

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Fission products

127I

126Te

130Te129Xe128Te

126Cd

126Ag

128Cd

127In

127Cd

127Ag

128Sn

128In

130Sn129Sn

129In

125Te

e.g. 126Ag(β-,n)125Cdvs 126Ag(β-)126Cd

Production of neutron-richradioactive isotopes in themass 80-130 range whichdecay by β- decay or by β-delayed neutron emissionBack to stable isotopes.Decay time scale dependsOn the associated half-liveswhich determine the fluxand time scale for delayedradiation exposure.

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Decline by the “rule of seven”This rule states that for every seven-fold increase in time following a fission detonation (starting at or after 1 hour), the radiation intensity decreases by a factor of 10. Thus after 7 hours, the residual fission radioactivity declines 90%, to one-tenth its level of 1 hour. After 7·7 hours (49 hours, approx. 2 days), the level drops again by 90%. After 7·2 days (2 weeks) it drops a further 90%; and so on for 14 weeks.

The rule is accurate to 25% for the first two weeks, and is accurate to a factorof two for the first six months. After 6 months, the rate of decline becomes much more rapid.

0.001

0.01

0.1

1

10

100

0.001 0.01 0.1 1.0 10.0 100.0 1000.0days

activ

ity (i

n %

)

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Studies of impact of ionizing radiation on the human body - Hiroshima -

US-Japanese teams medical tests, autopsies, human organ analysis, on-site radioactivity measurements …

autopsy

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Hiroshima radiation spread dataPrimary γ ray originated low dose of <100 rad near the hypocenter,secondary γ-ray originated dose of >100 rad within 1500 m radius

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Radiation Exposure Types

* *****

Irradiation Internal Contamination

External Contamination

*

*

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Schematic Model of Radionuclide Uptake

Intake:Intake: InhalationInhalation

LungLung

GIGITractTract

LymphLymphNodesNodes

SurfaceSurface

SkinSkin1. Intact1. Intact2. Wounds2. Wounds

IngestionIngestion

Lung ClearanceLung Clearance

BloodBlood

KidneyKidney Deposition SitesDeposition Sites

FecesFeces UrineUrine1. Whole Body1. Whole Body

2. Bone2. Bone3. Liver3. Liver

4. Thyroid4. Thyroid

Uptake:Uptake:

Excretion:Excretion:

(Recycle)(Recycle)

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Radiation interacting with cell molecules

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Linear energy transfer (LET): amount of energy deposited per unit track length

Energy dependence of radiation damage

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Human lethality as function of Dose

A 50% lethalityis reached at an accumulateddose of 450 cGy=450 rad=4.5 Gy.A 100 rad doseis survivable.

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Survival Chance

For people who died within 2 days to 2 monthsafter bomb explosion

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Radiation Side Effects radiation sickness

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Purpura, Vomiting, …

Purpura, or bleeding under the skin, is one of the symptoms of acute radiation sickness. The heavily exposed survivors experienced fever, nausea, vomiting, lack of appetite, bloody diarrhea, epilation, purpura, sores in their throat or mouth (nasopharyngeal ulcers), and decay and ulceration of the gums about the teeth (necrotic gingivitis). The time of onset of these symptoms depends on the exposure level.

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Long term effects - blindness

Radiation damage to epithelial Cells. Damaged cells move to the back of the eye and causelens opacity by blocking light.Occurs with 50% chance forpeople with dose of ~500 rad.

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Epilation – severe loss of hairHair loss is a common sign of radiation exposure & sickness.Severe epilation (2/3 hair loss) occurs at doses of >200 rad.

2km from hypocenter

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Hemogramblood impact of 300 rad exposure

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MO

RTA

LITY

RA

TE

( %

)

100 rad = 1 Gy ≈ 1 SvRadiation >2 Gy suppresses normal bone marrow functionsand causes long term mutationof red or white blood cells

Radiation impact on bone marrow

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LeukemiaWhen leukemia develops, the body produces large numbers of abnormal blood cells. In most types of leukemia, the abnormal cells are white blood cells.

An increase in the number of leukemia cases was first noted in the late 1940s. As of 1990, there were 176 leukemia deaths among 50,113 survivors with significant exposures (>0.5Gy). It is estimated that about 90 of these deaths are associated with radiation exposure.

Time (years)

Ris

k

Time radiation dose received

Latent periodPeriod at risk

Risk curve

0 4 30

Leukemia Latency and Time at Risk Periods

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Leukemia – case of Sadako

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Long range genetic effects

Chromosomes observed duringcell division. Abnormal ones aremarked by grey arrow.

Observed increase with doseindicates long term genetic effects