Muons from Neutralino Annihilations in the Sun: Flipped SU(5)

Details Muons from Neutralino Annihilations in the Sun: Flipped SU(5) Muons from Neutralino Annihilations in the Sun: Flipped SU(5)

2011-01-04

arxiv.org/abs/1101.0835v2

Phys.Rev.D83:075017,2011

Physics

High Energy Physics

High Energy Physics - Phenomenology

13 pages, 11 figures, 1 table

Scientific paper

10.1103/PhysRevD.83.075017

We consider two classes of supersymmetric flipped SU(5) models with gravity mediated supersymmetry breaking such that the thermal neutralino relic abundance provides the observed dark matter density in the universe. We estimate the muon flux induced by neutrinos that arise from neutralino annihilations in the Sun and discuss prospects for detecting this flux in the IceCube/Deep Core experiment. We also provide comparisons with the corresponding fluxes in the constrained minimal supersymmetric standard model and non-universal Higgs models. Regions in the parameter space that can be explored by the IceCube/DeepCore experiment are identified.

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