Annual Modulation Signature for the Direct Detection of Milky Way Wimps and Supergravity Models

Details Annual Modulation Signature for the Direct Detection of Milky Way Wimps and Supergravity Models Annual Modulation Signature for the Direct Detection of Milky Way Wimps and Supergravity Models

1999-02-03

arxiv.org/abs/hep-ph/9902237v1

Phys.Rev.D60:044002,1999

Physics

High Energy Physics

High Energy Physics - Phenomenology

14 pages, 5 figures

Scientific paper

10.1103/PhysRevD.60.044002

An analysis is given of the annual modulation signal for the direct detection of relic neutralinos within the framework of supergravity unified models. It is shown that both the minimal and the non-minimal SUGRA models can generate neutralino-proton cross-sections at the level compatible with the signals reported in the DAMA experiment at the Gran Sasso National Laboratory. Effects of proton stability on the analysis of the DAMA data in the minimal and the non-minimal SUGRA models are also discussed.

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