Interaction with matter...Formula needs to be modified for electrons Bethe-Bloch formula is not...
Transcript of Interaction with matter...Formula needs to be modified for electrons Bethe-Bloch formula is not...
Katharina Müller, Autumn 14 1
Understanding/description of interaction between matter and high energetic particles/radiationimportant:
● Principles of detection of particles/radiation
● Limitation of detectorsEfficiencyPosition resolutionEnergy resolutionTime resolution
● Impact on biological systemsRadiation damageRadiation protectionRadiation therapy
● Literature K. Kleinknecht, Teilchendetektoren
C. Grupen, Teilchendetektoren (BI Wissenschaftsverlag)
J. Ferbel, Experimental Techniques in High Energy Physics
Particle data group, chapter 26 , http://pdg.lbl.gov/pdg.html
The particle detector brief book http://rkb.home.cern.ch/rkb/titleD.html
dEdX: http://www.srim.org/SRIM/SRIMPICS/SRIM-High%20Velocity.pdf
Interaction with matter
Katharina Müller, Autumn 14 2
Interaction with matterEnergy loss per distance (dE/dx)
many different interactions, dominating processes depend on energy and particle type
Charged particles: defined reach
● Ionisation and excitation of electrons on shell→ Bethe-Bloch formula
● Coulomb Scattering: Scattering in Coulomb field of nucleussmall energy loss, but deflection
● Bremsstrahlung : dominant for low masses → radiation length
Photons: Absorption in matter, highly energy dependent – attenuation, no defined reach● Photo electrical effect● Compton scattering● Pair production
Hadrons: inelastic scattering ● Hadron+nucleus → π±,0 , K, p,n, fragments of nucleus
Z, A,
z, m, E, Θ
e± ,μ±, ± , , p,n,
Katharina Müller, Autumn 14 3
Energy loss of charged particles in matterEnergy loss due to ionisation and excitation
Energy loss per distance (dE/dx) : many theoretical works
● N. Bohr Classical derivation
● Bethe, Bloch Quantum mechanical description
● L. Landau Charge distribution function
● E. Fermi Density correction
...
Katharina Müller, Autumn 14 4
Ionisation: classical derivation (Bohr)Energy loss via inelastic collisions with electrons on shell → Ionisation and excitation
Assumptions: M(particle) >> me
Shell electron at rest (collision time small wrt orbital time)Projectile M, v = βc , charge ze, Target: charge Ze
Energy transfer onto target with mass mt: ΔE=Δp/(2m
t)
Momentum transfer: time integral
longitudinal forces cancel
only transversal forces important
p=∫−∞
∞
FCoulomb dt FC=1
40zZe2
/r2
F t=FC⋅b∣r∣
=FC⋅cos
F l x =−F l−x
Z e
r b
x
4
b: collision parameter
ze
Katharina Müller, Autumn 14 5
Ionisation: classical derivation (Bohr) I
Transversal forces on projectile
Momentum transfer onto target
Integration →
Energy transfer onto target with mass mt
Now: Sum over all shell electrons Integration over all collision parameters b
p b=∫−∞
∞
FC t dt=∫−∞
∞
FC tdxv=
140
z Z e2
b2 ∫−∞
∞
cos3dx
b d /cos2
v
FC t=1
40
z Z e2
r2˙cos=
140
z Z e2
b2˙cos3
E b= p2
2 mt
=2 z2 e4
me c2
2 b21
40
≡1
shell electron Z = 1, mt=m
e
1/m: collisions with nucleus may be neglected
=1
40
z Z e2
b v ∫−/2
/2
cosd =1
40
2 z Z e2
b v
r=b/cosθ
Katharina Müller, Autumn 14 6
Ionisation: classical derivation (Bohr) IIEnergy loss due to collisions with electrons in tube (length dx, thickness db) at radius b:
# of electrons: 2 π b db dx Ne electron density Ne = NA Z/A ρ
(NA Avogadro's constant, A mass number)
Integration over collision parameter from bmin to bmax
maximal energy transfer: central collision
minimal energy transfer: mean excitation energy I (averaged excitation potential per electron in the target)
−dE b= E bN e dV=4 z2 e4
me c2
2N e
dbb
dx
−dEdx
b=4 z2 e4
me c2
2N A
ZA
1b
db −dEdx
=4 z2 e4
me c2
2 N A
ZA
lnbmax
bmin
E b=22 me 2 c2
=2 z2 e4
me c2 2 b2
bmin=z e2
me c2
2
bmax=z e2
c 2
me I
b
db
dx
note: 1/β2
Katharina Müller, Autumn 14 7
(dE/dx) classical derivation (Bohr) III
Classical formula for energy loss due to ionisation
Unit [dE/dx] = MeV /cm
Warning: usually energy loss is divided by density: [dE/dX] = MeV cm2/g
→ dE/dX almost independent of material only material dependence through Z/A and ln(1/I)
−dEdx
=4 z2 e4
me c2
2N A
ZA
lnbmax
bmin
bmin=z e2
me c2
2bmax=
z e2
c 2me I
−dEdx
=K z2
2
ZA
12
ln2c2
2
2 me
IK=
4 e4
c2 me
N A=0.31 MeV cm2/g
Katharina Müller, Autumn 14 8
(dE/dx) Bethe Bloch Formula
full quantum mechanical derivation: Bethe-Bloch Formula
I mean excitation energyZ atomic numberA mass number of absorberValidity: 6 MeV < E < 6 GeV (π), generally 0.02< β<0.99 (1% accuracy!!)
T max: max kinematic energy transferred
z: Charge of particle dE/dX ∝ z2
Corrections
● δ(β) Density correction due to polarisation, important for high energies● C/Z Correction close to shell boundaries, relevant for small energies 1% @ βγ =0.3
−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T max
I 2−
2−
2−
CZ]
K=4 e4
c2 me
N A=0.31 MeV cm2/g
Katharina Müller, Autumn 14 9
(dE/dx) Bethe-Bloch-(Sternheimer) Formulaclassical result:
full quantum mechanical derivation: Bethe-Bloch Formula
describes mean energy loss or stopping power
●T max: max kinematic energy transferred from particle (M) onto electron
● small energies and particles with high masses: result equals classical result except factor 2 (imperfect description of very far collisions : binding of electrons cannot be neglected)
● independent of mass of particle ! (γm e<<M)● Unit MeV/(g/cm2) dx = ρ ds is material occupancy● dE/dX almost independent of target material● Formula needs to be modified for electrons ● Bethe-Bloch formula is not valid for slow particles βγ<0.02 where dE/dX ∝ β
−dEdX
=K z2
2
ZA
12
ln2 me c2 2 2
I
−dEdX
=K z2 ZA
1β2
[12
ln2 me c2β2γ2T max
I 2−β2−δ
2−
CZ]
T max=2 me c222
12 me/Mme /M 2
≈ 2 me c2
2
2me≪M
9
≈ M c2∞
Katharina Müller, Autumn 14 10
Energy loss dE/dX
Titel
dE/dx of muons in copper
~β
~1/β2
~2 ln(γβ)
● βγ < 3 dE/dX ∝ 1/β2
● βγ ≃ 3.5 minimum dE/dX 1-1.7 MeV cm2/g
● βγ > 3.5 logarithmic rise dE/dX ≃ 2 MeV cm2/g● βγ > 1000 Bremsstrahlung
dominant● very low energy: BB not valid,
empirical models● low energies: shell corrections● high energies: density corr.
Minimum: βγ 3-4 minimum ionising particle (MIP) looses ~ 1-1.7 MeV/(g/cm2)
PDG http://pdg.lbl.gov/pdg.html
Katharina Müller, Autumn 14 11
Shell correction−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T max
I 2−
2−
2−
CZ]
● Shell corrections (C/Z) constitute a correction to slow particles (e.g for protons in the energy range of 1-100 MeV)
● Correction for the assumption that particle velo-city >> bound electron velocity
● Assumption that electron is at rest not valid
● Maximal about 6%
● Calculation with various approximations
● J. F. Ziegler, Applied Physics Reviews / J. Applied Phys-ics, 85, 1249-1272 (1999).
● http://www.srim.org/SRIM/SRIMPICS/IONIZ.htm
Copper: about 1% at βγ=0.3 (6 MeV Pion), decreases rapidly with velocity
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Mean excitation energy I−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T max
I 2−
2−
2−
CZ]
I characteristic for target material I = 16 Z 0.9 eV for Z > 1
I=10 eV·Z for Z>20
Example Argon: Z = 18, I = 215 eV, measured 190.8 eV (Ionisation energy 15.7eV)
Mean excitation energy > ionisation E Theoretical calculation of I has a long history. Summaries can be found in several reviews :U. Fano, Chr., Studies in Penetration of Charged Particles in Matter, Nucl. Sci. Rpt.. 39, U. S. National Academy of Sciences, Washington, 1-338 (1964). J. F. Ziegler, “Handbook of Stopping Cross-Sections for Energetic Ions in All Elements”, Pergamon Press (1980).
PDG http://pdg.lbl.gov/pdg.html
Katharina Müller, Autumn 14 13
Charge dependence−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T max
I 2−
2−
2−
CZ]
Tracks of ions in emulsion
Iron Z = 26 Thorium Z = 90
Energy loss depends quadraticallyon charge of projectilewidth allows estimate of charge
Katharina Müller, Autumn 14 14
dE/dX discussion
● depends on velocity not on mass → particle identification
● βγ small dE/dx ∝ 1/β2
● βγ ≅ 3.5 broad minimum light absorbers: Z/A ≃ 0.5 ● dE/dx(min) ≃ 1.5 MeV /(g/cm2)
→ minimal ionising particles (MIP)
● βγ > 4 dE/dx ∝ 2 ln(βγ2) logarithmic (relativistic) rise
1/2
MIP
≅ 3-4
without
T max≈2 me c2 22
relativistic rise
−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T max
I 2−
2−
2−
CZ]
Katharina Müller, Autumn 14 15
dE/dxmin different materials
dE/dX depends on A, Z of target material
βγ≅ 3.5 broad minimum → minimum ionising particles (MIP)
H2 Z/A≅ 1 dE/dXmin ≅ 4 MeV /(g/cm2)others Z/A≅ 0.5 dE/dXmin ≅ 2 MeV /(g/cm2)
dE/dXmin ≅ 1-1.7 MeV /(g/cm2) only weak material dependence
PDG http://pdg.lbl.gov/pdg.html
−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T max
I 2−
2−
2−
CZ]
Katharina Müller, Autumn 14 16
dE/dX at minimumβγ → 3.5 broad minimum dE/dXmin ≅ 1-1.7 MeV/(g/cm2)only small material dependence
dE/dX(min) for different chemical elements fitted by a straight line Z>6
PDG http://pdg.lbl.gov/pdg.html
Katharina Müller, Autumn 14 17
Relativistic RiseLorentz-contraction of field linestransversal component of E-field grows with γ → larger collision distances, more collisions
Saturation for high energies→ Fermi plateau Tmax
= E
Solids (dE/dX)β→1≈ 1.05-1.1 (dE/dX)MIP
Gases (dE/dX)β→1≈ 1.5 (dE/dX)MIP
δ-correction, density effect:E-field gets partially shielded for high densities due to polar-isation δ(γ) = 2 ln γ +ζ (ζ material constant)→ less collisions with far distant electrons, smaller dE/dX
Fermi plateauwithout correction
with correction
at rest
E- field
Katharina Müller, Autumn 14 18
Particle identification
dE/dx only depends on velocity not on mass of particle → Particle identification
−dEdx
≈K z2 ZA
1
2[ ln
2 me c2
2
2
I−
2−
2−
CZ] as long as 2me≪M
ALICE TPC measured energy loss
• Heavy particles dE/dx well described by Bethe-Bloch formula
• Electrons not described by Bethe-Bloch
http://aliceinfo.cern.ch/
Katharina Müller, Autumn 14 19
ALICE TPC
88 m3 cylinder filled with gas, 5.1 m long
Divided in two drift regions by the central electrode located at its axial centre.
Uniform electric field along the z-axis electrons drift towards the end plates
Signal amplification:avalanche effect near anode wires
Readout: 570132 pads in cathode of multi-wire proportional chamber
http://aliceinfo.cern.ch/Public/en/Chapter2/Chap2_TPC.html Cosmic muon in TPC
Katharina Müller, Autumn 14 20
Restricted Bethe BlochParticle detectors don't measure energy loss, but energy deposited in detector.
Eg. highly energetic electrons may leave the detector → measured energy is too small
Restricted Bethe Bloch: Cut off parameter Tcut
:dE with T>Tcut
are neglected
Tupper
= min(Tcut
,Tmax
)
−dEdX
=K z2 ZA
1
2[12
ln2 me c2
2
2 T upper
I 2−
21
T upper
T cut
−
2−
CZ]
Katharina Müller, Autumn 14 21
Range in mattermean range R/M (M mass of particle)
Formally: integration of Bethe-Bloch formula
statistical process → mean penetration depthrange in cm: divided by density!
Example 1 GeV particle in leadK+ M= 493.6 MeV βγ = 2.02 → R/M = 800 g cm-2 GeV-1
R = 395 g cm-2
ds = R= 35 cm in lead
Myon R/M = 7000 g cm-2 GeV-1 ds = 64 cm
Proton R/m = 220 g cm-2 GeV-1 ds = 18 cm
R=∫E
0dXdE
dE
PDG http://pdg.lbl.gov/pdg.html
Katharina Müller, Autumn 14 22
Ionisation tracksEnergy loss largest for low energy particles → increase of energy deposits (ionisation) towards end of range (Bragg peak)
δ-(knock-on) electrons: have high enough energy for ionisation track
Tracks of mono energetic α particles in cloud cham-ber: range 8.6 cm, small variation
Katharina Müller, Autumn 14 23
Range: Bragg curveBragg curve: describes energy loss of particle as function of penetration depth
Particle in matter → particle de-accelerates→ energy loss increases as particle gets slower
Bragg-Peak: largest energy deposit at end of the trackimportant for radiation therapy!
Penetration depth
70 MeV protons in water
Charged particles
Photons
Bragg peak
Katharina Müller, Autumn 14 24
Medicine: radiation therapy
Possible to precisely deposit dose at well defined depth by varying beam energy
Application in medicine:Concentration of energy deposit at end of reach allows treatment of tumours with moderate exposure dose for the surrounding tissue, contrary to x-ray
Ionisation profile for 12C ions in water
Katharina Müller, Autumn 14 25
Proton therapy at PSI
Spread out Bragg peaks (SOBP)Different absorbers → almost constant dose in region of tumour
Katharina Müller, Autumn 14 26
Energy loss (Straggling)
Energy loss is statistical process N: number of collisions● ionisation loss distributed statistically● collisions with small dE more probable● large dE rare → electrons with keV (δ-electrons)● δ-rays have enough energy for ionisation● asymmetry: mean energy loss > most probable energy loss
Parametrisation: asymmetric Landau distribution
Landau-Tail: rare interactions with large energy transfer Tails up to the kinematic maximum
Bethe-Bloch gives mean energy loss
Thick layers or dense material: Gaussian distr.
dEdX: most probable value ≠mean energy loss
Δ E=∑i=0
Nδ E i
En
erg
y loss
pro
bab
ility
Energy loss
Katharina Müller, Autumn 14 27
Landau distributionMeasurement
ΔEmp =82 keV ΔEmp = 56.5 keV
Landau: Probability (Δ E) =
ξ: material constant mean energy loss in layer x ξ= K ρ x /β2 depends on density, thickness and velocityΔ E mean E- loss, Δ Emp most probable E-loss
12
exp−12e−
= E− E mp/
Katharina Müller, Autumn 14 28
δ Electrons
Energy distribution of secondary electrons:
(Spin 0)
d N 2
dT d x=12k z 2
ZA1
2F T
T 2
Example: 500 MeV pion in 300 μm Si: 5% produce an electron with T>166 keVimportant background in Cherenkov counterNumber of δ-electrons proportional z2/β2
F T =1−2T /T max
Katharina Müller, Autumn 14 29
δ Electrons
Number of δ electrons proportional to z2/β2
1969 Mc Cusker: Evidence of quarks in air shower cores (Phys Rev Lett)Narrow tracks in cloud chambers: low ionisation→ charge < 1!
Katharina Müller, Autumn 14 30
Summary dE/dx through ionisationdescribed by Bethe-Bloch Formula
● only small material dependence
● Energy loss ∝ z2 (particle)
● independent of mass → particle identification
● most of the energy is deposited towards the end of the range
● βγ < 3 dE/dX ∝ 1/β2
● βγ ≃ 3.5 minimum dE/dX 1-1.7 MeV cm2/g
● βγ > 3.5 logarithmic rise dE/dX ≃ 2 MeV cm2/g
● βγ > 1000 Bremsstrahlung dominant
● Bethe-Bloch is not valid for slow particles (βγ<0.05) (dE/dX ∝ β) here only phenomenological models available
Katharina Müller, Autumn 14 31
Additional Material: Ranges
Range of electrons, protons and α particles in air and water
Katharina Müller, Autumn 14 32
Additional Material: Ionisation yield
Material Density g/cm3 Eion
[eV] I[eV] W[eV] np [cm-1] n
t [cm-1]
H2
8.99 10-5 15.4 19.2 37 5.2 9.2He 1.78 10-4 24.5 41.8 41 5.9 7.8N
21.25 10-3 15.6 82 35 10 56
Ne 9.00 10-4 21.6 137 36 12 39Ar 1.78 10-3 15.7 188 26 29 94Xe 5.89 10-3 12.1 482 22 44 307C4H
102.67 10-3 10.8 48.3 23 46 195
Ar-f 1.4 15.4 188 29.6 98000Xe-f 3.06 12.1 482 15.6 245000Si 2.33 3.6 172 1000000
● W = E/nt mean energy per electron-ion pair
● np Primary ionisation: directly produced electron-ion pairs ~ 1.45 Z
● nT= n
P +secondary ionisation: add. electron-ion pairs through primary electrons
● W: mean energy for production of electron-ion pair● W higher than ionisation energy
● Semiconductors, W small, many electron-ion pairs, good resolution, small detectors
Katharina Müller, Autumn 14 33
Additional material: dE/dX: Mixtures
Since BB applies to pure elements, direct measurements are needed in compounds for accurate values.Good approximation: weighted sum of loss rates of constituentsweighted according to fraction a
i of electrons
1dEd x
=∑ w i
idEd x
i
w i=a i A iA e ff
Z e ff=∑ a i Z iA e ff=∑ a i A i
ai is the molar fraction of element i with atomic weight A
i,
Aeff
is the atomic weight of all constituents
Tables for density and shell correction