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Gravitino dark matter and general neutralino NLSP

L. Covi et al JHEP11(2009)003   doi: 10.1088/1126-6708/2009/11/003  Help

Open Access This is an Open Access article.

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L. Covia, J. Hasenkampa,b, S. Pokorskic and J. Robertsd
a Deutsches Elektronen-Synchrotron DESY, Hamburg, Germany
b Institute for Theoretical Physics, Hamburg University, Hamburg, Germany
c Institute of Theoretical Physics, Warsaw University, Warsaw, Poland
d Center for Cosmology and Particle Physics, New York University, New York, NY 10003, U.S.A.
E-mail: Laura.Covi@desy.de, Jasper.Hasenkamp@desy.de, Stefan.Pokorski@fuw.edu.pl and Jonathan.Roberts@nyu.edu

Abstract. We study the scenario of gravitino DM with a general neutralino NLSP in a model independent way. We consider all neutralino decay channels and compare them with the most recent BBN constraints. We check how those bounds are relaxed for a Higgsino or a Wino NLSP in comparison to the Bino neutralino case and look for possible loopholes in the general MSSM parameter space. We determine constraints on the gravitino and neutralino NLSP mass and comment on the possibility of detecting these scenarios at colliders.

Key words: Cosmology of Theories beyond the SM; Supersymmetric Standard Model

E-print number: 0908.3399
Cited: by
Refers: to

Received 4 September 2009, accepted for publication 8 October 2009
Published 4 November 2009

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