Strong lensing by fermionic dark matter in galaxies
It has been shown that a self-gravitating system of massive keV fermions in thermodynamic equilibrium correctly describes the dark matter (DM) distribution in galactic halos (from dwarf to spiral and elliptical galaxies) and that, at the same time, it predicts a denser quantum core towards the cente...
Guardado en:
| Autores principales: | Gómez, Gabriel L., Argüelles, Carlos Raúl, Perlick, Volker, Rueda, Jorge A., Ruffini, Remo |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2016
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/99493 https://ri.conicet.gov.ar/11336/55240 https://journals.aps.org/prd/abstract/10.1103/PhysRevD.94.123004 https://arxiv.org/abs/1610.03442 |
| Aporte de: |
Ejemplares similares
-
Galaxy rotation curves and universal scaling relations: comparison between
phenomenological and fermionic dark matter profiles
por: Krut, A., et al.
Publicado: (2023) -
Can fermionic dark matter mimic supermassive black holes?
por: Argüelles, Carlos Raúl, et al.
Publicado: (2019) -
Dark matter response to galaxy assembly history
por: Artale, M.C., et al. -
Dark matter response to galaxy assembly history
Publicado: (2019) -
The impact of baryons on dark matter haloes
por: Pedrosa, S., et al.