28 citations · 100 across the 7 of their papers we have counts for
5 papers
Galaxy Rotation Curve Fitting Using Machine Learning Tools
Carlos R. Argüelles, Santiago Collazo
Galaxy rotation curve (RC) fitting is an important technique which allows the placement of constraints on different kinds of dark matter (DM) halo models. In the case of non-phenom…
On the growth of supermassive black holes formed from the gravitational collapse of fermionic dark matter cores
C. R. Argüelles, K. Boshkayev, A. Krut +5
Observations support the idea that supermassive black holes (SMBHs) power the emission at the center of active galaxies. However, contrary to stellar-mass BHs, there is a poor unde…
Fermionic Dark Matter: Physics, Astrophysics, and Cosmology
C. R. Argüelles, E. A. Becerra-Vergara, J. A. Rueda +1
The nature of dark matter (DM) is one of the most relevant questions in modern astrophysics. We present a brief overview of recent results that inquire into a possible fermionic qu…
Galaxy rotation curves and universal scaling relations: comparison between phenomenological and fermionic dark matter profiles
A. Krut, C. R. Argüelles, P. -H. Chavanis +2
Galaxies show different halo scaling relations such as the Radial Acceleration Relation, the Mass Discrepancy Acceleration Relation (MDAR) or the dark matter Surface Density Relati…
Strong lensing by fermionic dark matter in galaxies
L. Gabriel Gómez, C. R. Argüelles, Volker Perlick +2
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 and pr…