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arxiv: astro-ph/0306561 · v1 · pith:PKGU5PUTnew · submitted 2003-06-26 · 🌌 astro-ph

Neutralino annihilation gamma-rays from clumps and the LMC

classification 🌌 astro-ph
keywords annihilationclumpsneutralinocloudclumpdarkdetectabilitydiscuss
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We discuss the detectability of dark matter clumps in the Milky Way halo due to neutralino annihilation. We then focus on a known ``clump'', the Large Magellanic Cloud.

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