| Issue |
EPJ Web Conf.
Volume 136, 2017
RICAP16, 6th Roma International Conference on Astroparticle Physics
|
|
|---|---|---|
| Article Number | 01002 | |
| Number of page(s) | 6 | |
| DOI | https://doi.org/10.1051/epjconf/201713601002 | |
| Published online | 23 March 2017 | |
https://doi.org/10.1051/epjconf/201713601002
Models of Supersymmetry for Dark Matter
1 Departamento de Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, E-28049 Madrid, Spain
2 Instituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, E-28049 Madrid, Spain
a e-mail: c.munoz@uam.es
Published online: 29 March 2017
A brief review of supersymmetric models and their candidates for dark matter is carried out. The neutralino is a WIMP candidate in the MSSM where R-parity is conserved, but this model has the μ problem. There are natural solutions to this problem that necessarily introduce new structure beyond the MSSM, including new candidates for dark matter. In particular, in an extension of the NMSSM, the right-handed sneutrino can be used for this job. In R-parity violating models such as the μvSSM, the gravitino can be the dark matter, and could be detected by its decay products in gamma-ray experiments.
© The Authors, published by EDP Sciences, 2017
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