The Phenomenology of Gravitino Dark Matter Scenarios in Supergravity Models

Details The Phenomenology of Gravitino Dark Matter Scenarios in Supergravity Models The Phenomenology of Gravitino Dark Matter Scenarios in Supergravity Models

2009-03-16

arxiv.org/abs/0903.2860v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, contributed to the proceedings of the Seventh International Heidelberg Conference on Dark Matter in Astro and Partic

Scientific paper

We review the phenomenology of gravitino dark matter within supergravity framework. Gravitino can be dark matter if it is the lightest supersymmetric particle, which is stable if R-parity is conserved. There are several distinct scenarios depending on what the next to lightest supersymmetric particle (NLSP) is. We discuss the constraints and summarize the phenomenology of neutralino, stau, stop and sneutrino NLSPs.

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