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The role of self-interacting right-handed neutrinos in galactic structure
We show that warm dark matter keV fermions (`inos') can be responsible for both core and halo galactic structure, in agreement with current astrophysical/cosmological constraints. We identify the inos with sterile right-handed neutrinos. The possible mass range of up to a few tens of keV, obtai...
Autores principales: | Argüelles, C.R., Mavromatos, N.E., Rueda, J.A., Ruffini, R. |
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Lenguaje: | eng |
Publicado: |
2015
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2016/04/038 http://cds.cern.ch/record/1984522 |
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