72 citations · 298 across the 15 of their papers we have counts for
15 papers
Thermodynamics of self-gravitating fermions as a robust theory for dark matter halos: Stability analysis applied to the Milky Way
A. Krut, C. R. Argüelles, P. -H. Chavanis
We present a framework for dark matter (DM) halo formation based on a kinetic theory of self-gravitating fermions together with a solid connection to thermodynamics. Based on maxim…
Modelling the Track of the GD-1 Stellar Stream Inside a Host with a Fermionic Dark Matter Core-Halo Distribution
Martín F. Mestre, Carlos R. Argüelles, Daniel D. Carpintero +2
Traditional studies on stellar streams typically involve phenomenological CDM halos or ad hoc dark matter (DM) profiles with different degrees of triaxiality, which preclude to…
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…
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…
The Role of Self Interactions in the Cosmological Evolution of Warm Dark Matter
Rafael Ignacio Yunis, Carlos R. Argüelles, Diana López Nacir +3
In this work we present a summary of recent studies on the effects of elastic self interactions in the evolution of Warm Dark Matter models (WDM), focusing on structure formation a…
Reshaping our understanding on structure formation with the quantum nature of the dark matter
Carlos R. Argüelles, Eduar A. Becerra-Vergara, Andreas Krut +3
We study the non-linear structure formation in cosmology accounting for the quantum nature of the dark matter (DM) particles in the initial conditions at decoupling, as well as in…