Neutralino Dark Matter from Indirect Detection Revisited

Simple item page
dc.creatorGrajek, Phill
dc.creatorKane, Gordon
dc.creatorPhalen, Daniel J.
dc.creatorPierce, Aaron
dc.creatorWatson, Scott
dc.date2008-07-09
dc.date2008-10-16
dc.date.accessioned2026-07-07T10:10:09Z
dc.date.available2026-07-07T10:10:09Z
dc.descriptionWe revisit indirect detection possibilities for neutralino dark matter, emphasizing the complementary roles of different approaches. While thermally produced dark matter often requires large astrophysical "boost factors" to observe antimatter signals, the physically motivated alternative of non-thermal dark matter can naturally provide interesting signals, for example from light wino or Higgsino dark matter. After a brief review of cosmic ray propagation, we discuss signals for positrons, antiprotons, synchrotron radiation and gamma rays from wino annihilation in the galactic halo, and examine their phenomenology. For pure wino dark matter relevant to the LHC, PAMELA and GLAST should report signals.
dc.description23 pages, 9 figures: v2. Corrected typos, fixed synchrotron bounds in light of bugs in program
dc.identifierhttps://arxiv.org/abs/0807.1508
dc.identifierhttp://arxiv.org/abs/0807.1508
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/171532
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleNeutralino Dark Matter from Indirect Detection Revisited
dc.typetext

Files

Collections

arXiv