passage of radiation through matter - universitetet i oslofolk.uio.no/gryt/leo2_matter.pdf ·...
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FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation 1
Passage of radiation through matter
- Important for detectors, shielding, nuclear medicine - Quantities: energy loss, scattering, straggling, absorption etc.
Cross section • Probability that a reaction takes place • dσ = ”area” of target • Ns = number scattered / sec
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€
dσdΩ(E,Ω) =
1FdNs
dΩdΩ = sinθdθdϕ
dΩ = 4π∫∫θ = 0 −πϕ = 0 − 2π
€
θ
€
ϕ
Point of interaction
Total cross section
3
€
σ(E) = dσ∫ = dΩ∫ dσdΩ
= sinθdθdϕ0
2π
∫0
π
∫ dσdΩ(E,θ,ϕ)
€
σ(E) = sinθdθdϕ0
2π
∫0
π
∫ dσdΩ(E) = 4π dσ
dΩ(E)
Isotropic scattering:
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Real life
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Target
€
Ns(Ω) = FA⋅ NδxdσdΩ
€
(Ntot = FA⋅ Nδxσ)
Number of centres seen
Number of scattered Particles into dΩ
Incident number of particles
Prob. of interaction
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Mean free path
5
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Probability of not having interaction between x - > x +dxP(x + dx) = P(x)(1− wdx)
P(x) +dPdx
dx = P − Pwdx
dP = −wPdxP = exp(−wx) Probability of survival from 0 - > x
Probability of suffering an interaction anywhere in the distance x :Pint (x) =1− exp(−wx)
Mean free path :
λ =xPdx∫Pdx∫
=1w
=1Nσ
€
P(x) : Probability of not having interaction between 0 - > xwdx : Probability of having interaction between x - > x + dx
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Target thickness
6 €
Physical thickness :
m = ρV = ρdA⇒ d =mAρ
[um]
Mass thickness :
t =mA
[mg/cm2]
A
d
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Main types
7
• Direct ionizing radiation E(x), I=const – α-particles – β – Protons – Heavy ions (20Ne, 40Ar, etc.)
• Indirect ionizing radiation E=const, I (x) – Neutrons – ν, π, Κ etc – γ, X-rays
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γ–ray attenuation coeff. (µ/t)
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Heavy charged particles
9
-dE/dx Bragg- toppen
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Bohr’s calculations
10
• Electron initially free and at rest • Trajectory not disturbed by the electron • Passing time so short that electron do
not move
ze b
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Momentum transfer (I)
11
Electric field:
Perpendicular momentum transfer:
Gauss’ law:
€
E(r) =ze
4πε 0r2
€
pper = eEperdt−∞
+∞
∫ =eEper
vdx =
ev−∞
+∞
∫ Eperdx−∞
∞
∫
€
! E ⋅ d! S = q
ε 0S∫
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Momentum transfer (II)
12
Integral over cylinder:
Perpendicular momentum transfer:
€
Eper−∞
+∞
∫ 2πbdx =zeε 0
€
pper =ze2
2πε 0bv
b db
x
Eper E
FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation 12
Energy transfer
FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation 13
€
ε =pper2
2me
=z2e4
8π 2ε 02b2mev
2
But a lot of electrons within db and dx:
€
N ⋅ dV = N ⋅ 2πb⋅ db⋅ dx
Energy transferred to projectile:
€
−dE = εNdV =z2e4N
8π 2ε02mev
22πbdbb2
dx
dx
db b
Stopping power
14
Integrating over impact parameter b:
€
−dEdx
=z2e4N
4πε02mev
2dbb
=bmin
bmax
∫ z2e4N4πε0
2mev2 ln
bmaxbmin
Naively:
€
bmin = 0bmax = ∞
FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation 14
Discussion bmin and bmax
15
electron
€
Δpmax = 2mev
εmax =Δp2max2me
= 2mev2
€
ε =z2e4
8π 2ε02b2mev
2 < εmax = 2mev2 ⇒ bmin =
14πε0
ze2
mev2
Short passage time t compared to electron period T:
v b
€
vt = b⇒ t =bv
< T =1ν ⇒ bmax =
vν
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Bohr’s classical formula
16
€
−dEdx
=z2e4N
4πε 02mev
2 ln
vν
14πε 0
ze2
mev2
=z2e4N
4πε 02mev
2 ln4πε 0mev
3
ν ze2
All essential features Relativistic by including γ in last term:
€
−dEdx
=z2e4N
4πε 02mev
2 ln 4πε 0γ2mev
3
ν ze2 , γ 2 =1− vc'
( ) *
+ ,
2
€
eCGS2 →
eSI2
4πε 0To transfer formulas in Leo from CGS ->SI unit system: 16 FYS-KJM5920 - Nuclear Measurement Methods and
Instrumentation
Bethe-Bloch’s formula
17
€
−dEdx
= 2πNare2mec
2ρZAz2
β2ln2meγ
2v 2Wmax
I2'
( )
*
+ , − 2β2 −δ − 2
CZ
.
/ 0
1
2 3
The stopping power of aluminium for protons
17 FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation
Thin target or absorber
18
E0 E1
θ
N(E)
N(θ)
0
E1 E0
ΔE Straggling
Scattering
E
θ
FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation 18
Range
19
€
R(E0) =dEdx
"
# $
%
& '
0
E 0
∫−1
dE
Roughly
€
−dEdx
∝ β−2 ∝ E −1
R(E0)∝ EdE0
E 0
∫ ∝ E02
2200 um
80 MeV FYS-KJM5920 - Nuclear Measurement Methods and
Instrumentation 19
Bragg-profiles
20
12C in water 4He in air
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21
Dagsavisen 27.1.2008
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22
0 5 10 15 20 Dybde [cm]
Relativ dose
γ fra 60Co
0
1
2
3
4
12C-ioner 250 MeV/u
18 MeV røntgen
Dosedistribution 12C versus X-rays
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23
Raster scan
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Particle telescope
24
ΔE E
Etot = E + ΔE ΔE
E
Low Etot High Etot
Punch through
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Bananas
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Bananas (60Ni-exp)
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Thickness of ΔE detector
27
Rα(E) (um)
E (MeV)
ΔE E
40MeV
5 MeV 35 MeV
35 40
700 550
d D - d
D = R(40) = 700um D-d = R(35) = 550um d = 700-550 = 150um
α
27 FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation
Thickness spectrum
28
If we used range curve Rα(E), other particles than α’s will “lie” about the thickness of the front detector ΔE p d t
3He α
17
24
31 106 129
N(d)
d (um)
€
ΔEd
≈dEdx
∝z2
v 2 ∝z2ME
Energy deposited in d for a given E is :ΔE ∝ z2M
FYS-KJM5920 - Nuclear Measurement Methods and Instrumentation 28