Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, 1 Aldo Morselli Andrea Lionetto Vladimir Zdravkovic.

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Presentation transcript:

Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, 1 Aldo Morselli Andrea Lionetto Vladimir Zdravkovic INFN, Sezione di Roma 2 & Università di Roma Tor Vergata Vladimir Zdravkovic INFN, Sezione di Roma 2 & Università di Roma Tor Vergata Search for Dark Matter with GLAST & PAMELA 5 th International Workshop on the Identification of Dark Matter 6th - 10th September th - 10th September 2004

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Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, 17 MASS 89

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Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, 38 Cangaroo Hess Cangaroo consistent with ~ 2 TeV M Hess > 12 TeV M Whipple HESS Coll. astro-ph/

Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, 39 Conclusions GLAST will explore a good portion of the supersymmetric parameter space … and this is only an additional item for GLAST !

Aldo Morselli, INFN, Sezione di Roma 2 & Università di Roma Tor Vergata, 40 GLAST will be an important step in gamma ray astronomy ( ~ sources compared to ~ 200 of EGRET) A partnership between High Energy Physics and Astrophysics Beam test and software development well on the way Wide range of possible answers/discoveries Gold era for multiwavelenght studies 2 nd Conclusions