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Galactic Neutrino Analysis and Simulation: Unlocking Cosmic Mysteries

Explore galactic latitude and longitude neutrino distribution, SNR distribution, and neutrino flux on Earth. Objectives include benchmarking neutrino fluxes, diffusing galactic neutrinos, and accumulating point sources like SNR, GRB, and AGN. Drive advancements in Galactic dark matter detection through reconstruction and shape recognition. Utilize abundant computing power for comprehensive data analysis.

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Galactic Neutrino Analysis and Simulation: Unlocking Cosmic Mysteries

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  1. WP2Physics analysis and simulation Ressources People Objectives

  2. 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) Ressources People Objectives

  3. Galactic latitude Galactic longitude SNR distribution νμ+νμon Earth HN model E2 x Neutrino flux [particles MeV s-1 cm-2] HE model C model HEMN model Calibration Software Energy [MeV] • Time calibration (cf. WP 3) Objectives Benchmark neutrino fluxes • Diffuse flux of galactic neutrinos • (Egret, AMS, HESS) • Accumulation of point sources SNR, GRB, AGN • (HESS, VERITAS) • Galactic dark matter Detector geometries Reconstruction & Shape recognition Ressources People Objectives

  4. Resources Computing power • 150 - 3GHz CPU • each machine containing • 1GB RAM and 120Gb disk Ressources People Objectives

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