Novel constraints on fermionic dark matter from galactic observables I: The Milky Way
We have recently introduced a new model for the distribution of dark matter (DM) in galaxies based on a self-gravitating system of massive fermions at finite temperatures, the Ruffini–Argü elles–Rueda (RAR) model. We show that this model, for fermion masses in the keV range, explains the DM halo of...
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| Autores principales: | Argüelles, Carlos Raúl, Krut, A., Rueda, J. A., Ruffini, R. |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/95886 https://ri.conicet.gov.ar/11336/84185 https://arxiv.org/abs/1606.07040 |
| Aporte de: |
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