wp2 physics analysis and simulation
DESCRIPTION
WP2 Physics analysis and simulation. Ressources. People. Objectives. In few months…. Neil McCauley (AC) 2 post-docs 1(+) student. People involved. Current. Stella Bradbury (AC) Fabrice Jouvenot (PostDoc) Joachim Rose (AC) Lee Thompson (AC) Christos Touramanis (AC). - PowerPoint PPT PresentationTRANSCRIPT
Fabrice Jouvenot University of LiverpoolThe 11th of April 2006
WP2WP2Physics analysis and simulationPhysics analysis and simulation
People ObjectivesObjectives Ressources
Fabrice Jouvenot University of LiverpoolThe 11th of April 2006
People involvedPeople involved
• Stella Bradbury (AC)
• Fabrice Jouvenot (PostDoc)
• Joachim Rose (AC)
• Lee Thompson (AC)
• Christos Touramanis (AC)
Current
• Neil McCauley (AC)
• 2 post-docs
• 1(+) student
In few months…
People ObjectivesObjectives Ressources
Fabrice Jouvenot University of LiverpoolThe 11th of April 2006
Detector geometries
ObjectivesObjectives
People ObjectivesObjectives Ressources
• Diffuse flux of galactic neutrinos
(Egret, AMS, HESS)
• Accumulation of point sources SNR, GRB, AGN
(HESS, VERITAS)
• Galactic dark matter
Benchmark neutrino fluxes
νμ+ νμ on Earth
Energy [MeV]
E2 x
Ne
utr
ino
flu
x [
pa
rtic
les
Me
V s
-1 c
m-2]
HEMN model
C model
HE model
HN model
SNR distribution
Calibration Software
• Time calibration (cf. WP 3)
Reconstruction &
Shape recognitionGalactic longitude
Ga
lact
ic la
titu
de
Fabrice Jouvenot University of LiverpoolThe 11th of April 2006
ResourcesResources
People ObjectivesObjectives Ressources
• 150 - 3GHz CPU
each machine containing
1GB RAM and 120Gb disk
Computing power