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Interaction of Particles with Matter Alfons Weber CCLRC & University of Oxford Graduate Lecture 2004.

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Presentation on theme: "Interaction of Particles with Matter Alfons Weber CCLRC & University of Oxford Graduate Lecture 2004."— Presentation transcript:

1 Interaction of Particles with Matter Alfons Weber CCLRC & University of Oxford Graduate Lecture 2004

2 Nov 20042 Table of Contents Bethe-Bloch Formula Energy loss of heavy particles by Ionisation Multiple Scattering Change of particle direction in Matter Cerenkov Radiation Light emitted by particles travelling in dielectric materials Transition radiation Light emitted on traversing matter boundary

3 Nov 20043 Bethe-Bloch Formula Describes how heavy particles (m>>m e ) loose energy when travelling through material Exact theoretical treatment difficult Atomic excitations Screening Bulk effects Simplified derivation ala MPhys course Phenomenological description

4 Nov 20044 Bethe-Bloch (1) Consider particle of charge ze, passing a stationary charge Ze Assume Target is non-relativistic Target does not move Calculate Energy transferred to target (separate) ze Ze b r θ x y

5 Nov 20045 Bethe-Bloch (2) Force on projectile Change of momentum of target/projectile Energy transferred

6 Nov 20046 Bethe-Bloch (3) Consider α-particle scattering off Atom Mass of nucleus: M=A*m p Mass of electron:M=m e But energy transfer is Energy transfer to single electron is

7 Nov 20047 Bethe-Bloch (4) Energy transfer is determined by impact parameter b Integration over all impact parameters b db ze

8 Nov 20048 Bethe-Bloch (5) Calculate average energy loss There must be limit for E min and E max All the physics and material dependence is in the calculation of this quantities

9 Nov 20049 Bethe-Bloch (6) Simple approximations for From relativistic kinematics Inelastic collision Results in the following expression

10 Nov 200410 Bethe-Bloch (7) This was just a simplified derivation Incomplete Just to get an idea how it is done The (approximated) true answer is with ε screening correction of inner electrons δ density correction, because of polarisation in medium

11 Nov 200411 Energy Loss Function

12 Nov 200412 Average Ionisation Energy

13 Nov 200413 Density Correction Density Correction does depend on material with x = log 10 (p/M) C, δ 0, x 0 material dependant constants

14 Nov 200414 Different Materials (1)

15 Nov 200415 Different Materials (2)

16 Nov 200416 Particle Range/Stopping Power

17 Nov 200417 Application in Particle ID Energy loss as measured in tracking chamber Who is Who!

18 Nov 200418 Straggling (1) So far we have only discussed the mean energy loss Actual energy loss will scatter around the mean value Difficult to calculate parameterization exist in GEANT and some standalone software libraries From of distribution is important as energy loss distribution is often used for calibrating the detector

19 Nov 200419 Straggling (2) Simple parameterisation Landau function Better to use Vavilov distribution

20 Nov 200420 Straggling (3)

21 Nov 200421 δ-Rays Energy loss distribution is not Gaussian around mean. In rare cases a lot of energy is transferred to a single electron If one excludes δ-rays, the average energy loss changes Equivalent of changing E max δ-Ray

22 Nov 200422 Restricted dE/dx Some detector only measure energy loss up to a certain upper limit E cut Truncated mean measurement δ-rays leaving the detector

23 Nov 200423 Electrons Electrons are different  light Bremsstrahlung Pair production

24 Nov 200424 Multiple Scattering Particles don’t only loose energy … … they also change direction

25 Nov 200425 MS Theory Average scattering angle is roughly Gaussian for small deflection angles With Angular distributions are given by

26 Nov 200426 Correlations Multiple scattering and dE/dx are normally treated to be independent from each Not true large scatter  large energy transfer small scatter  small energy transfer Detailed calculation is difficult but possible Wade Allison & John Cobb are the experts

27 Nov 200427 Correlations (W. Allison) Example: Calculated cross section for 500MeV/c  in Argon gas. Note that this is a Log-log-log plot - the cross section varies over 20 and more decades! log k L 2 18 17 7 log k T whole atoms at low Q 2 (dipole region) electrons at high Q 2 electrons backwards in CM nuclear small angle scattering (suppressed by screening) nuclear backward scattering in CM (suppressed by nuclear form factor) Log p L or energy transfer (16 decades) Log p T transfer (10 decades) Log cross section (30 decades)

28 Nov 200428 Signals from Particles in Matter Signals in particle detectors are mainly due to ionisation Gas chambers Silicon detectors Scintillators Direct light emission by particles travelling faster than the speed of light in a medium Cherenkov radiation Similar, but not identical Transition radiation

29 Nov 200429 Cherenkov Radiation (1) Moving charge in matter at rest slow fast

30 Nov 200430 Wave front comes out at certain angle That’s the trivial result! Cherenkov Radiation (2)

31 Nov 200431 Cherenkov Radiation (3) How many Cherenkov photons are detected?

32 Nov 200432 Different Cherenkov Detectors Threshold Detectors Yes/No on whether the speed is β>1/n Differential Detectors β max > β > β min Ring-Imaging Detectors Measure β

33 Nov 200433 Threshold Counter Particle travel through radiator Cherenkov radiation

34 Nov 200434 Differential Detectors Will reflect light onto PMT for certain angles only  β Selecton

35 Nov 200435 Ring Imaging Detectors (1)

36 Nov 200436 Ring Imaging Detectors (2)

37 Nov 200437 Ring Imaging Detectors (3) More clever geometries are possible Two radiators  One photon detector

38 Nov 200438 Transition Radiation Transition radiation is produced when a relativistic particle traverses an inhomogeneous medium Boundary between different materials with different n. Strange effect What is generating the radiation? Accelerated charges

39 Nov 200439 Initially observer sees nothing Later he seems to see two charges moving apart  electrical dipole Accelerated charge is creating radiation Transition Radiation (2)

40 Nov 200440 Transition Radiation (3) Consider relativistic particle traversing a boundary from material (1) to material (2) Total energy radiated Can be used to measure γ

41 Nov 200441 Transition Radiation Detector

42 Nov 200442 Table of Contents Bethe-Bloch Formula Energy loss of heavy particles by Ionisation Multiple Scattering Change of particle direction in Matter Cerenkov Radiation Light emitted by particles travelling in dielectric materials Transition radiation Light emitted on traversing matter boundary

43 Nov 200443 Bibliography PDG 2004 (chapter 27 & 28) and references therein Especially Rossi Lecture notes of Chris Booth, Sheffield http://www.shef.ac.uk/physics/teaching/phy311 R. Bock, Particle Detector Brief Book http://rkb.home.cern.ch/rkb/PH14pp/node1.html Or just it!

44 Nov 200444 Plea I need feedback! Questions What was good? What was bad? What was missing? More detailed derivations? More detectors? More… Less… A.Weber@rl.ac.uk


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