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Seminario Geant4 INFN

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Title: Seminario Geant4 INFN


1
Precision Validation of Geant4 Electromagnetic
Physics
Susanna Guatelli Barbara Mascialino
G.A.P. Cirrone (INFN LNS), G. Cuttone (INFN LNS),
S. Donadio (INFN,Genova), S. Guatelli (INFN
Genova) , M. Maire (LAPP), A. Mantero (ESA) , B.
Mascialino (INFN Genova), P. Nieminen (ESA), L.
Pandola(INFN LNGS), S. Parlati (INFN LNGS) , A.
Pfeiffer (CERN), M.G. Pia (INFN Genova), L. Urban
(Budapest)
1st Workshop on Italy-Japan Collaboration on
Geant4 Medical Application
2
Electromagnetic Physics
  • It handles
  • electrons and positrons
  • gamma, X-ray and optical photons
  • muons
  • charged hadrons
  • ions
  • multiple scattering
  • Bremsstrahlung
  • ionisation
  • annihilation
  • photoelectric effect
  • Compton scattering
  • Rayleigh effect
  • gamma conversion
  • ee- pair production
  • synchrotron radiation
  • transition radiation
  • Cherenkov
  • refraction
  • reflection
  • absorption
  • scintillation
  • fluorescence
  • Auger

3
E.M. Physics Validation
  • Validation is fundamental in Geant4
  • Validations at different levels
  • Comparisons to experimental measurements and
    recognised standard references
  • Unit, integration, system testing
  • Microscopic physics validation
  • Macroscopic validation experimental use cases

4
Microscopic Validation
  • Validation of Geant4 electromagnetic physics
    models
  • Attenuation coefficients, CSDA ranges, Stopping
    Power, distributions of physics quantities
  • Quantitative comparisons to experimental data and
    recognised standard references

5
Photon Mass Attenuation Coefficient
x-ray attenuation coeff in U
NIST data Penelope
c219.3 n22 p0.63
Absorber Materials Be, Al, Si, Ge, Fe, Cs, Au,
Pb, U
6
X-ray Attenuation Coefficient - Al
7
X-ray Attenuation Coefficient - Al
?2N-P15.9 ?19 p0.66
8
X-ray Attenuation Coefficient - Ge
9
X-ray Attenuation Coefficient - Ge
?2N-P10.1 ?21 - p0.98
10
X-ray Attenuation Coefficient - U
11
X-ray Attenuation Coefficient - U
?2N-P19.3 ?22 - p0.63
12
Compton Scattering - Al
13
Compton Scattering - Al
?2N-P2.5 ?6 - p0.87
14
Compton Scattering - Cs
15
Compton Scattering - Cs
?2N-P4.6 ?8 - p0.80
16
Rayleigh Scattering - Al
?2N-L13.6 ?11 - p0.26
17
Rayleigh Scattering - Al
?2N-P7.2 ?8 - p0.52
18
Rayleigh Scattering - Cs
19
Rayleigh Scattering - Cs
20
Photoelectric Effect - Fe
21
Photoelectric Effect - Fe
22
Pair Production - Si
23
Pair Production - Si
24
Electrons - Stopping Power and CSDA Range
G4 Standard G4 LowE-EPDL NIST
Absorber Materials Be, Al, Si, Ge, Fe, Cs, Au,
Pb, U
G4 Standard G4 LowE-EPDL NIST
CSDA range particle range without energy loss
fluctuations and multiple scattering
Experimental set-up
centre
25
Electrons - CSDA Range - Al
26
Electrons - CSDA Range - Pb
27
Electrons - Stopping Power - Al
28
Electrons - Stopping Power - Pb
29
Electrons - CSDA Range Al G4LowE
Regression testing
30
Electrons - CSDA Range Pb G4Standard
Regression testing
31
Protons - CSDA Range Al
32
Protons - CSDA Range Pb
33
Protons - Stopping Power Al
34
Protons - Stopping Power - Pb
35
Protons - CSDA Range Al G4LowE
Regression testing
36
Protons - CSDA Range Al G4LowE Ziegler
Regression testing
37
Protons - CSDA Range Al G4Standard
Regression testing
38
Protons - CSDA Range Pb G4LowE
Regression testing
39
Protons - CSDA Range Pb G4LowE Ziegler
Regression testing
40
Protons - CSDA Range Pb G4Standard
Regression testing
41
Electrons Transmission Tests
Experimental set-up
e- beam
42
Electrons Backscattering Coefficient E100keV
Backscattered e-
Experimental set-up
Incident e- beam
Angle of incidence (with respect to the normal
to the sample surface) 0
43
Electrons Backscattering Coefficient E1MeV
Angle of incidence (with respect to the normal
to the sample surface)0
44
Positrons - Backscattering coefficient 30keV
45
Positrons - Backscattering coefficient 30keV
Regression testing
46
Auger Effect, X-Ray Fluorescence
Anderson-Darling Test Ac (95) 0.752
Detector response
Simulation of Auger emission from pure materials
irradiated by an electron beam with continuous
spectrum
47
Much more available or in progress
ions
Barkas Effect
48
Macroscopic Validation
  • Experimental set-up validation
  • Collaboration of Geant4 developers
  • and research groups of different experiments

Medical Physics
Space science
49
The Problem of Validation Finding Reliable Data
Note Geant4 validation is not always
easy experimental data often exhibit large
differences!
Backscattering low energies - Au
50
Conclusions
  • Geant4 electromagnetic package encompasses an
    ample set of physics models, specialised for
    particle type, energy range and detector
    applications
  • Geant4 Physics Reference Manual
    (www.cern.ch/geant4)
  • Geant4 e.m. physics is subject to a rigorous
    testing and validation process
  • Many detailed results are available for the
    validation of basic physics distributions
  • (http//www.ge.infn.it/geant4/analysis/test)
  • Many significant contributions to the validation
    of Geant4 e.m. physics from test beams and
    application in the experiments

51
Geant4 Physics Book
  • A project has been recently launched for a Geant4
    Physics Book
  • To have a solid and comprehensive reference on
    Geant4 physics
  • Collaborative effort involving Geant4 physics
    groups, experiments
  • Main focus of the project is Geant4 physics
    models validation

Collaboration with detector experts valuable and
welcome!
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