Are two kinds of dark matter seen in Galactic gamma rays?

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dc.creatorRoos, Matts
dc.date2005-01-04
dc.date2005-01-10
dc.date.accessioned2026-07-07T02:16:38Z
dc.date.available2026-07-07T02:16:38Z
dc.descriptionExcesses of Galactic gamma rays in the 1-100 GeV region observed by EGRET and by WMAP have been interpreted as signals of dark matter (LSP) annihilation. We argue that the excess of TeV gamma rays from the Galactic center observed by H.E.S.S. signals a heavier dark matter component with a very small relic density.
dc.description2 pages, no figures, RevTex4. Missing text header inserted, three new references added
dc.identifierhttps://arxiv.org/abs/astro-ph/0501055
dc.identifierhttp://arxiv.org/abs/astro-ph/0501055
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8860
dc.subjectAstrophysics
dc.titleAre two kinds of dark matter seen in Galactic gamma rays?
dc.typetext

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