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Interaction of Particles with Matter

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Presentation on theme: "Interaction of Particles with Matter"— Presentation transcript:

1 Interaction of Particles with Matter
Alfons Weber STFC & University of Oxford Graduate Lecture 2009

2 Table of Contents Bethe-Bloch Formula Multiple Scattering
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 Dec 2009 Alfons Weber

3 For which detectors is energy loss important? Dec 2009 Alfons Weber

4 Bethe-Bloch Formula Describes how heavy particles (m>>me) loose energy when travelling through material Exact theoretical treatment difficult Atomic excitations Screening Bulk effects Simplified derivation ala MPhys course Phenomenological description Dec 2009 Alfons Weber

5 Bethe-Bloch (1) Consider particle of charge ze, passing a stationary charge Ze Assume Target is non-relativistic Target does not move Calculate Momentum transfer Energy transferred to target ze b y r θ x Ze X or Y? Dec 2009 Alfons Weber

6 Bethe-Bloch (2) Efficient target? Force on projectile
Change of momentum of target/projectile Energy transferred Efficient target? Dec 2009 Alfons Weber

7 Bethe-Bloch (3) Consider α-particle scattering off Atom
Mass of nucleus: M=A*mp Mass of electron: M=me But energy transfer is Energy transfer to single electron is Dec 2009 Alfons Weber

8 Bethe-Bloch (4) Energy transfer is determined by impact parameter b
Integration over all impact parameters b db ze Dec 2009 Alfons Weber

9 Bethe-Bloch (5) Calculate average energy loss There must be limits
material dependence is in the calculation of the limits Dec 2009 Alfons Weber

10 Bethe-Bloch (6) Simple approximations for
From relativistic kinematics Inelastic collision Results in the following expression Dec 2009 Alfons Weber

11 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 (polarisation in medium) Dec 2009 Alfons Weber

12 Energy Loss Function Dec 2009 Alfons Weber

13 Average Ionisation Energy
Dec 2009 Alfons Weber

14 Density Correction Density Correction does depend on material with
x = log10(p/M) C, δ0, x0 material dependant constants Dec 2009 Alfons Weber

15 Different Materials (1)
Dec 2009 Alfons Weber

16 Different Materials (2)
Dec 2009 Alfons Weber

17 Particle Range/Stopping Power
Dec 2009 Alfons Weber

18 Energy-loss in Tracking Chamber
Who is who? Dec 2009 Alfons Weber

19 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 Dec 2009 Alfons Weber

20 Straggling (2) Simple parameterisation Landau function
Better to use Vavilov distribution Dec 2009 Alfons Weber

21 Straggling (3) Dec 2009 Alfons Weber

22 δ-Ray 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 Emax δ-Ray Dec 2009 Alfons Weber

23 Restricted dE/dx Some detector only measure energy loss up to a certain upper limit Ecut Truncated mean measurement δ-rays leaving the detector Dec 2009 Alfons Weber

24 Electrons Electrons are different light Bremsstrahlung
Pair production Dec 2009 Alfons Weber

25 More next time... Dec 2009 Alfons Weber

26 Multiple Scattering Particles don’t only loose energy … … they also change direction Dec 2009 Alfons Weber

27 MS Theory Average scattering angle is roughly Gaussian for small deflection angles With Angular distributions are given by Dec 2009 Alfons Weber

28 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 Dec 2009 Alfons Weber

29 Correlations (W. Allison)
nuclear small angle scattering (suppressed by screening) nuclear backward scattering in CM (suppressed by nuclear form factor) electrons at high Q2 whole atoms at low Q2 (dipole region) Log cross section (30 decades) log kL 2 18 17 7 log kT Log pL or energy transfer (16 decades) electrons backwards in CM 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 pT transfer (10 decades) Dec 2009 Alfons Weber

30 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 Dec 2009 Alfons Weber

31 Cherenkov Radiation Moving charge in dielectric medium
Wave front comes out at certain angle slow fast Dec 2009 Alfons Weber

32 Cherenkov Radiation (2)
How many Cherenkov photons are detected? Dec 2009 Alfons Weber

33 Different Cherenkov Detectors
Threshold Detectors Yes/No on whether the speed is β>1/n Differential Detectors βmax > β > βmin Ring-Imaging Detectors Measure β Dec 2009 Alfons Weber

34 Threshold Counter Particle travel through radiator Cherenkov radiation
Dec 2009 Alfons Weber

35 Differential Detectors
Will reflect light onto PMT for certain angles only  β Selection Dec 2009 Alfons Weber

36 Ring Imaging Detectors (1)
Dec 2009 Alfons Weber

37 Ring Imaging Detectors (2)
Dec 2009 Alfons Weber

38 Ring Imaging Detectors (3)
More clever geometries are possible Two radiators  One photon detector Dec 2009 Alfons Weber

39 Transition Radiation Transition radiation is produced, when a relativistic particle traverses an inhomogeneous medium Boundary between different materials with different diffractive index n. Strange effect What is generating the radiation? Accelerated charges Dec 2009 Alfons Weber

40 Transition Radiation (2)
Before the charge crosses the surface, apparent charge q1 with apparent transverse vel v1 After the charge crosses the surface, apparent charges q2 and q3 with apparent transverse vel v2 and v3 Dec 2009 Alfons Weber

41 Transition Radiation (3)
Consider relativistic particle traversing a boundary from material (1) to material (2) Total energy radiated Can be used to measure γ Dec 2009 Alfons Weber

42 Transition Radiation Detector
Dec 2009 Alfons Weber

43 ATLAS TRTracker ATLAS Experiment Inner Detector:
pixel, silicon and straw tubes Combination of Central Tracker and TR for electron identification Dec 2009 Alfons Weber

44 Atlas TRT (II) Dec 2009 Alfons Weber

45 Electrons with radiator Electrons without radiator
Atlas TRT (III) only electron produce TR in radiator e± / π separation Electrons with radiator Electrons without radiator Bod -> J/yKos TRT senses ionisation transition radiation High threshold hits Dec 2009 Alfons Weber

46 Table of Contents Bethe-Bloch Formula Multiple Scattering
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 Dec 2009 Alfons Weber

47 Bibliography This lecture
PDG 2008 (chapter 27 & 28) and references therein Especially Rossi Lecture notes of Chris Booth, Sheffield R. Bock, Particle Detector Brief Book Or just it! Dec 2009 Alfons Weber

48 Plea I need feedback! Questions Alfons.Weber@stfc.ac.uk What was good?
What was bad? What was missing? More detailed derivations? More detectors? More… Less… Dec 2009 Alfons Weber


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