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Radiation interaction with matter
1
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Outline
Introduction
Generalities cross section
dE/dx
LET and NIEL
Proton
electrons
range, practical range
Ionising and non ionising dose
Conclusion
2
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Particles of interest
h
Photonsx,
protons[1MeV, 1GeV]
electrons[10keV, 10 MeV]
ions[1 MeV/uma, 1 GeV/uma]
3
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GENERAL : Energy loss by unit path length
4
dx
Interaction
dE
E - dEEdE
dx
Assuming a straight line trajectory
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Nature of the medium
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
SiSi
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
Si
e-
e-
e-
silicium
Incident particle
CoulombicScattering
v
v
v
Incident particle
Nuclear Reaction
Slo
win
g do
wn
5,4 A0,9 A
a) b)
Slo
win
g do
wn
Electrons act as a viscous medium that slow down incident particle
In addition, the probability to encounter a nuclei is not nul
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Ionisation and Displacement for charged particles
interaction with electrons
- ionisation- Coulombic inelastic
scattering
interaction with nuclei
- displacements - elastic scattering
- nuclear reaction
vacancy
interstitial
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Total stopping power 9
Not negligeable for energetic electronin heavy material
Not negligeable for low energy protons
e-nucleus Bremsstrahlung
NIEL + phonon Ionising stopping power
electronicnuclearTotal dx
dE
dx
dE
dx
dE
rayelectronicnuclearTotal dx
dE
dx
dE
dx
dE
dx
dE
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slowing down of particles
Proton stopping power
Unit : MeV/m or MeV/mg.cm2
12
1.E+01
1.E+02
1.E+03
1.E+04
1.E+05
1.E-02 1.E-01 1.E+00 1.E+01 1.E+02
Energy (MeV)
LE
T (
Me
V/g
.cm
2 )
Proton
Silicium
Lithium
Ions in Silicon
Bragg Peak
dE/dx is proportional to density
dE/dx is maximal when incident & target particle are identical
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slowing down of particlesStopping power of electrons
1.E+00
1.E+01
1.E+02
1.E-02 1.E-01 1.E+00 1.E+01
Energy (MeV)
LE
T (
Me
V/g
.cm
2 )
Hydrogen
Aluminium
Lead
Electrons
Bragg Peak
dE/dx is proportional to specific gravity
dE/dx is maximal when incident & target particle are identical
13
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14
Displacement damages
P
interstitial
vacancy
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Protons
E
1 eV
0,1 MeV
1 MeV
188 eV
10 MeV
No more displacementRecoil energy < 25 eV
Elastic scattering- Coulombic scattering- nuclear scattering
Nuclear reaction
21
In silicon
P
Slow
ing down by ionisation
displacement
P
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Interaction of Charged particles with matter : electrons
- rays emissionBremsstrahlung
E
1 MeV
250 keV
No more displacementRecoil energy < 25 eV
- Coulombic scattering
Gamma
Some displacements
22
Slow
ing down by ionisation
In silicon
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Bremsstrahlung : Interaction of electromagnetic radiation with matter
- rays E
10-3 eV
m
1 eV
3 eV
100 eV
1 MeV
1 mm
750 nm
400 nm
10 nm
1 pm
23
Gamma ray emission by interaction with electric field of the atom of thetarget
Zincident Ztarget
Mincident
I 2
negligeable
large Mincident
Proton Electron
Heavy material
with large Ztarget
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Range of particles
The range is deduced from the stopping power
dE
dxdE
Erange 1
)(
24
range
depth
Al
1 MeV electron beam
0
40
80
120
0 0.5 1 1.5 2Dif
fere
nti
al p
ath
len
gth
d
istr
ibu
tio
n
range
practical range
0
20
40
60
80
100
0 0.5 1 1.5 2Aluminum thickness [mm]
Tran
smis
sio
n r
ate
(%)
Inte
gra
ted
pat
h l
eng
th
dis
trib
uti
on
1 MeV electron in Al rangepractical range
mean crossed thickness
Al27
13
Mat
eria
l sur
face
Range > depthMean penetration depth
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Range of protons & ions
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E-03 1.E-02 1.E-01 1.E+00 1.E+01 1.E+02
Energy (MeV)
Ran
ge (
g/cm
2 )
hydrogen
aluminum
lead
Protons
25
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E-02 1.E-01 1.E+00 1.E+01 1.E+02
Energy (MeV)
Ra
ng
es
(g/c
m2 )
Proton
Silicon
Lithium
Ions in Silicion
Ions in siliconProtons in different materials
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Range of electrons
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E-02 1.E-01 1.E+00 1.E+01 1.E+02 1.E+03
Energie (MeV)
Par
cour
s (g
/cm
2 )
hydrogen
aluminum
lead
Electrons
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0.001
0.01
0.1
1
10
100
0.01 0.1 1 10
Energy (MeV)A
lum
inum
thic
knes
s (m
m)
Practical range
Practical range (10% transmissionrate)Mean crossed thickness (50%transmission rate)Range
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Order of magnitude27
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trajectories28
Aluminium Proton (100 MeV)
Aluminium
Electrons (1 MeV)
Back-scattered electron
10 MeV electrons in AlBremsstrahlung
100 MeV protons in Al
84 MeV Carbon in Silicon
1 MeV electrons in Al
1E-10
1E-09
1E-08
1E-07
1E-06
1E-05
1E-04
1E-03
1E-02
1E-01
1E+00
0 18 36 54 72 89 107 125 143 161 179 197 215 233 251 268 286 304 322 340 358 363
thickness (µm)
ray
(g/c
m²)
Trace d'un ion carbone de 150 MeV dans du silicium
direction de l'ion
150 MeV 5 MeV
1E+14
1E+16
1E+19
3E+20 4E+20 5E+20 1E+21
5,99 µm
90 MeV
2 E+20
8 E+20
3 E
+21
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Ionising and non ionising dose29
Dose is the averaged energy deposited by unit of mass :
J/ kg = Gray1 Gray = 100 rad
Flux
dx
Deposited energy E
Surface S atoms/cm3
dn scattered particles
Volume Mass
Incident Number of particle
LETdx
dE
dxS
dESDose
1
. NIEL
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Ionising Dose : Normaly incident protons
0
200
400
600
800
1000
1200
0.00001 0.0001 0.001 0.01 0.1 1
Thickness (g/cm2)
Do
se
(G
ray
)
30 kev
150 keV 400 keVdose for 10+10p/cm2
1 MeV
10 MeV
30
Due to straggling andscattering
Compromise betweenthe increase of the LET and the decrease of the flux due to scattering
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Al
0
40
80
120
0 0.5 1 1.5 2Dif
fere
nti
al
pa
th l
en
gth
dis
trib
uti
on
range
practical range
0
20
40
60
80
100
0 0.5 1 1.5 2Aluminum thickness [mm]
Tra
ns
mis
sio
n r
ate
(%
)
Inte
gra
ted
path
le
ng
th
dis
trib
uti
on
1 MeV electron in Al rangepractical range
mean crossed thickness
Al2713
Mat
eria
l sur
face
0.0
1.0
2.0
3.0
4.0
5.0
6.0
7.0
8.0
0.0 0.2 0.4 0.6 0.8 1.0 1.2
THICKNESS Al (g/cm2)
2,5 MeV
2,0 MeV
1,5 MeV
1,0 MeV
0,6 MeV
ELECTRONS IN ALUMINUM
(1E10 e/cm2 - normal incidence)
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Ionising Dose : Normaly incident electrons
Peack smoother than for protonsas electrons arelargely scattered
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Electrons, incidence 30deg, 400keV,in aliminum
1.E-06
1.E-05
1.E-04
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
0.00001 0.0001 0.001 0.01 0.1 1 10 100 1000
Thickness (mm)
Do
se
(G
y)
densite = 2.7 g/cm3
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Ionising Dose : Normaly incident electrons + Bremsstrahlung
Bragg Peak
Dose enhancementga
mm
a
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Mission ionising dose : LEO, GEO33
LEO ORBIT (Spot)Infinite slab
1.E-03
1.E-02
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.E+04
1.E+05
1E-5 1E-4 1E-3 1E-2 1E-1 1E+0 1E+1 1E+2
Thickness Al (g/cm2)
DO
SE
Al (
Gra
ys/y
ear)
Total
Trapped protons, AP8Min
Solar flare Protons, Feynman Min
Trapped electrons, AE8Min
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.E+04
1.E+05
1.E+06
1.E+07
1.E+08
1E-05 0.0001 0.001 0.01 0.1 1 10 100 1000
Thickness (mm)D
ose
Al (
Gy/
year
)
Solar flare protons
Trapped electrons
Trapped protons
GEO ORBITSolar maximum
Infinite Slab
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YEAR AVERAGED DOSE FOR GPS ORBIT
1.E-01
1.E+00
1.E+01
1.E+02
1.E+03
1.E+04
1.E+05
1.E+06
0.001 0.01 0.1 1 10 100
THICKNESS Al (g/cm2)
GEANT, AE8Min : électrons
Orbit : 20000 km, 55° - Solar Minimum
GEANT 4 calculationDouble infinite slab
34
Mission ionising dose : GPS
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Conclusion37
Electron act as a viscous medium that slow down incident charged particles
Interaction with electron produce ionisation (LET)
Interaction with nuclei produce displacement (NIEL)
Ionising and non ionising dose (Energy deposited by unit of mass)
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Conclusion38
LET is used to quantify SEE effects (SEU(LET))
NIEL is used to quantify degradation of optoelectronic components
Dose is used to quantify degradation of electronic devices ( MOS, Bipolar)
LET, NIEL and dose are the fondemental parameters used to quantifymany degradations induced by space radiations