The role of self-interacting right-handed neutrinos in galactic structure
It has been shown previously that the DM in galactic halos can be explained by a self-gravitating system of massive keV fermions ('inos') in thermodynamic equilibrium, and predicted the existence of a denser quantum core of inos towards the center of galaxies. In this article we show that...
Guardado en:
| Autores principales: | Argüelles, Carlos Raúl, Mavromatos, N. E., Rueda, J. A., Ruffini, R. |
|---|---|
| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2016
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/101748 https://ri.conicet.gov.ar/11336/54357 http://iopscience.iop.org/article/10.1088/1475-7516/2016/04/038/meta https://arxiv.org/abs/1502.00136 |
| Aporte de: |
Ejemplares similares
-
Galactic Center constraints on self-interacting sterile neutrinos from fermionic dark matter ("ino") models
por: Yunis, Rafael, et al.
Publicado: (2020) -
Galaxy rotation curve fitting using machine learning tools
por: Argüelles, Carlos Raúl, et al.
Publicado: (2023) -
The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations
por: Ishiyama, Tomoaki, et al.
Publicado: (2021) -
The effects of galactic winds on the chemical evolution of baryons
por: De Rossi, M.E., et al. -
The effects of galactic winds on the chemical evolution of baryons
Publicado: (2009)