Supersymmetric Dark Matter after LHC Run 1

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Different mechanisms operate in various regions of the MSSM parameter space to bring the relic density of the lightest neutralino, neutralino_1, assumed here to be the LSP and thus the Dark Matter (DM) particle, into the range allowed by astrophysics and cosmology. These mechanisms include coannihil...

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Detalles Bibliográficos
Autores principales: Bagnaschi, E.A., Buchmueller, O., Cavanaugh, R., Citron, M., De Roeck, A., Dolan, M.J., Ellis, J.R., Flächer, H., Heinemeyer, S., Isidori, G., Malik, S., Martínez Santos, D., Olive, K.A., Sakurai, K., de Vries, K.J., Weiglein, G.
Lenguaje:eng
Publicado: 2015
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1140/epjc/s10052-015-3718-9
http://cds.cern.ch/record/2040986

Internet

https://dx.doi.org/10.1140/epjc/s10052-015-3718-9
http://cds.cern.ch/record/2040986

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