Search for Dark Matter with GLAST

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dc.creatorMorselli, Aldo
dc.creatorLionetto, Andrea
dc.creatorCesarini, Alessandro
dc.creatorFucito, Francesco
dc.creatorUllio, Piero
dc.date2002-11-14
dc.date2003-05-05
dc.date.accessioned2026-07-07T10:31:26Z
dc.date.available2026-07-07T10:31:26Z
dc.descriptionThe detection of exotic cosmic rays due to pair annihilation of dark matter particles in the Milky Way halo is a viable techniques to search for supersymmetric dark matter candidates. The study of the spectrum of gamma-rays, antiprotons and positrons offers good possibilities to perform this search in a significant portion of the Minimal Supersymmetric Standard Model parameter space. In particular the EGRET team have seen a convincing signal for a strong excess of emission from the Galactic center that has no simple explanation with standard processes. We will review the limits achievable with the experiment GLAST taking into accounts the LEP results and we will compare this method with the antiproton and positrons experiments.
dc.description8 pages, 12 figures, Invited talk at the First International Workshop on Fundamental and Particle Physics in Space, Space Part, May 14-19 2002, Isola d'Elba. V2: one figure updated, references added
dc.identifierhttps://arxiv.org/abs/astro-ph/0211327
dc.identifierhttp://arxiv.org/abs/astro-ph/0211327
dc.identifierNucl.Phys.Proc.Suppl.113:213-220,2002
dc.identifierdoi:10.1016/S0920-5632(02)01844-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178412
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSearch for Dark Matter with GLAST
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