Simulation and Analysis for Astroparticle Experiments

Slides:



Advertisements
Similar presentations
A particle monitor for LISA Pathfinder and Gravity Probe-B gyroscope charging in LEO Peter Wass, Henrique Araújo, Tim Sumner Imperial College London, UK.
Advertisements

Institut für Kernphysik Markus Horn ILIAS-N3, BSNS-working group meeting Valencia, Forschungszentrum Karlsruhe in der Helmholtz-Gemeinschaft.
EAS EXPERIMENT ON BOARD OF THE AIRBUS A380 J. N. Capdevielle, F. Cohen, PCC, College de France K. Jedrzejczak, B. Szabelska, J. Szabelski, T. Wibig The.
Cosmic rays in solar system By: Tiva Sharifi. Cosmic ray The earth atmosphere is bombarded with the energetic particles originating from the outer space.
Hadronic and Electromagnetic Physics: special applications V.Ivanchenko BINP, Novosibirsk, Russia & CERN, Geneve, Switzerland.
Alex Howard Imperial College Geant4 Users Workshop, CERN, 13 th November 2002 LowE EM PartII 1 Low Energy Electromagnetic Physics PART II Alex Howard.
PLANETOCOSMICS L. Desorgher, M. Gurtner, E.O. Flückiger, and P. Nieminen Physikalisches Institut, University of Bern ESA/ESTEC.
Centre de Toulouse Radiation interaction with matter 1.
NEEP 541 Radiation Interactions Fall 2003 Jake Blanchard.
30 September 2002Geant4 Workshop, CERN1 ESA Geant4 Activities ESA Space Environment & Effects Analysis Section P. Nieminen, E. Daly, H.D.R. Evans, A. Keating,
Friday May 10th 2002 Alex Howard Imperial College LondonSlide 1 Experiences of Submitting UKDMC and LISA GEANT4 Jobs FIRST I should say thanks for the.
The PLANETOCOSMICS Geant4 application L. Desorgher Physikalisches Institut, University of Bern.
Hadronic Physics II Geant4 Users’ Tutorial CERN February 2010 Gunter Folger.
Monday June 3rd 2002 AIDA 2.2 WorkshopAlex Howard Imperial College London Slide 1 Implementation of AIDA within Geant4 for Underground and Space Applications.
David Argento (some aspects of) cosmogenic nuclide production.
20 September 1999Geant4 Workshop1 in Space : Examples of Past and Future Missions and Experiments P. Nieminen, ESA/ESTEC, The Netherlands.
Gamma Flux Bubble Chamber Expected Rates – Sept 2015 January 20,
Dose Predictions for Moon Astronauts Image Source: Nicholas Bachmann, Ian Rittersdorf Nuclear Engineering and Radiological Sciences.
1 Giuseppe G. Daquino 26 th January 2005 SoFTware Development for Experiments Group Physics Department, CERN Background radiation studies using Geant4.
Alex Howard, CERN Slide 1 Simulating Dark Matter Detectors (a.k.a. DMX Underground Advanced Example) 1.Dark Matter detectors 2.Implementation within Geant4.
Alex Howard, Imperial College Slide 1 July 2 nd 2001 Underground Project UNDERGROUND PROJECT – Overview and Goals Alex Howard Imperial College, London.
Nuclear Chemistry. Reactions All the reactions you have see have involved transfer or share of electrons. The atoms on the left are the same as the atoms.
Some nuclei – usually large ones – are unstable They cannot fit their neutrons and protons into a space small enough that that strong nuclear force can.
A radioactive isotope is an atom that has a nucleus that is not stable (will change to form a nucleus of a different element). The process by which the.
24 th October 2002 Alex Howard, Imperial College, London 8 th TopIcal Seminar on Innovative Radiation and Particle Detectors Slide1 Simulation and Analysis.
Cosmic Ray Composition Primary cosmic particles collide with atoms in the Earth's atmosphere and produce a cascade of short lived particles, which can.
Comparisons of neutron production by muons in GEANT4 and toy model
Geant4 Simulation of Test-Mass Charging in the LISA Mission
Solar gamma-ray and neutron registration capabilities of the GRIS instrument onboard the International Space Station Yu. A. Trofimov, Yu. D. Kotov, V.
Types of Radiation.
Validation of Geant4 against the TARC benchmark: Testing neutron production, transportation and interaction TARC – experimental set-up and aims Geant4.
INTERACTION OF PARTICLES WITH MATTER
Nuclear Radiation.
Project Structure Advanced Neutron Spectrometer on the International Space Station (ANS-ISS) Mark Christl NASA/MSFC Oct 23, 2015 Honolulu, HI 1 1.
Andrea Chiavassa Universita` degli Studi di Torino
Complete description of the 12C(n,n'3a) and 12C(n,a)9Be reactions in the High Precision neutron model A. R. Garcia, E. Mendoza and D. Cano-Ott Nuclear.
Gamma-ray Albedo of the Moon Igor V. Moskalenko (Stanford) & Troy A
PARTICLE FLUX CALCULATION-III
Neutron Detection with MoNA LISA
Phosphorescent materials continue to glow after the lights are turned off. How can you use the model of an atom to explain this?
proton mass, mp neutron mass, mn electron mass, me
Nuclear Chemistry Physical Science.
P. Nieminen, E. Daly, A. Mohammadzadeh, H.D.R. Evans, G. Santin
Particle Physics Part 1 -James Joyce Contents: Particle Accelerators
Russian Research Center “ Kurchatov Institute”
Radioactive Decay.
University of Delaware
Radioactive Decay.
Quantification of solar wind parameters from measurments by SOHO and DSCOVR spacecrafts during series of Interplanetary Coronal Mass Ejections in the.
Subatomic Particles and Quantum Theory
Radioactive Decay.
Hadronic Physics in Geant4
Summary of alpha etc.
Low Energy Electromagnetic Physics PART II
The Hadrontherapy Geant4 advanced example
Chapter 9 Nuclear Radiation
Ionising Radiation.
Nuclear Radiation Natural Radioactivity Nuclear Equations
Ionising Radiation.
NUCLEAR CHEMISTRY.
Radioactive Decay.
The mass numbers on the left and right of the equations must be equal.
Nuclear Fusion Nuclear Fission Gamma radiation Beta radiation
AN ORIGINAL MODEL FOR THE SIMULATION OF LOW ENERGY ANTIPROTONS
Nuclear Radiation Natural Radioactivity Nuclear Equations
1. Alpha decay of radium-226 with gamma emission
Radioactivity Chapter 18.
Gamma Decay: 23994Pu 23994Pu +  Nucleus has energy levels
Nuclear Radiation Natural Radioactivity Nuclear Equations
Unit 4 – Nuclear Reactions
Presentation transcript:

Simulation and Analysis for Astroparticle Experiments The LISA Gravitational Wave Interferometer Implementation within Geant4 Simulation output from the GRID and predictions Conclusions Future work Alex Howard, CERN Alex Howard, CERN Slide1

Geant4 Simulation of Test-Mass Charging in the LISA Mission   Very long base-line: 1 million km Very high precision: < 1nm – 1pm (!) Alex Howard, CERN Slide2

charge management system Test-Mass Charging charging rate fluctuations Lorentz + Coulomb forces p shielding charge management system Alex Howard, CERN Slide3

Geometry spacecraft payload area Alex Howard, CERN Slide4

LISA 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 Alex Howard, CERN Slide5

Physics List EM processes (LowE) Electrons, Gammas, etc Atomic de-excitation Hadrons (no hFluorescence) Hadronic processes Elastic (LE+HE) Inelastic (LE+HE) Nuclear de-excitation Absorption/Annihilation Photonuclear (g, e, m) Neutrons (HP, LE, HE) Decays Decay in flight (no RDM) Secondaries Cuts: (250 eV), 1um - 5um Kill e- outside caging Alex Howard, CERN Slide6

OUTPUT 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 Alex Howard, CERN Slide7

6secs and Convergence of Charging Rate Alex Howard, CERN Slide8

6secs and Convergence of Charging Rate Initial indications of charging rate Alex Howard, CERN Slide9

Results I Charging rate 2 days in parallel !!! G4 result: 58 +e/s 45 s exposure ~ 10,000,000 events 1 charging event ~ 2,000 events ~ 40,000 events/day/CPU 2 days in parallel !!! Charging rate G4 result: 58 +e/s (G3 result: 11 +e/s) 52 +e/s 6 +e/s Alex Howard, CERN Slide10

Results II Cuts (~0.1 um) 250 eV 52 +e/s 1 um 8.77 keV 41 +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! Alex Howard, CERN Slide11

Conclusions 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 Alex Howard, CERN Slide12