Title: Alex Howard, CERN Slide1
1Simulation and Analysis for Astroparticle
Experiments
- The LISA Gravitational Wave Interferometer
- Implementation within Geant4
- Simulation output from the GRID and predictions
- Conclusions
- Future work
2Geant4 Simulationof Test-Mass Chargingin the
LISA Mission
- Very long base-line
- 1 million km
- Very high precision
- lt 1nm 1pm (!)
3Test-Mass Charging
p
4Geometry
spacecraft
payload area
5LISA Environment
1. Protons from solar flares Localised in
time 2. Extragalactic cosmic rays Protons,
Alphas Isotropic flux MeV TeV
energies peak 500 MeV/nucleon
Jursa AS (ed) 1985
previous G3 simulations
Jafry et al. 1996, 1997
G4 simulation
6Physics List
EM processes (LowE) Electrons, Gammas, etc Atomic
de-excitation Hadrons (no hFluorescence)
Hadronic processes Elastic (LEHE) Inelastic
(LEHE) Nuclear de-excitation Absorption/Annihilat
ion Photonuclear (g, e, m) Neutrons (HP, LE, HE)
Decays Decay in flight (no RDM)
Secondaries Cuts (250 eV), 1um - 5um Kill e-
outside caging
7OUTPUT from Grid Running
- Over 100 jobs have been run on the grid to try
and estimate the charging rate in the proof mass
and test different cuts and processes within
Geant4. - 1.9 million events have been run in 300 hours of
CPU time
86secs and Convergence of Charging Rate
96secs and Convergence of Charging Rate
Initial indications of charging rate
10Results I
45 s exposure 10,000,000 events 1 charging
event 2,000 events 40,000 events/day/CPU
Charging rate
G4 result 58 e/s
(G3 result 11 e/s)
52 e/s
6 e/s
11Results II
Cuts
1 um 8.77 keV 41 e/s
(0.1 um) 250 eV 52 e/s
2 um 30.7 keV 40 e/s
5 um 53.2 keV 42 e/s
Energy of Primary, MeV
Decreasing the production threshold from 10 keV
(G3, G4EM) to 250 eV (G4LowE) leads to a 20
increase of the charging rate!
12Conclusions
- The LISA Gravitational Wave spacecraft has been
simulated in order to estimate the proof mass
charging due to the space environment - Charging rate increased 5 times relative to G3
simulation - more physics, wider primary energy, geometry and
lower cuts