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