activity
20242026
collaborators

7 papers

astro-ph.GA2026

Temporal Correlations Between Fuzzy Dark Matter and Baryonic Matter in Virialized Core-Halo Structures

Ivan Alvarez-Rios, Francisco S. Guzman

Fuzzy Dark Matter (FDM) predicts the existence of virialized halos with interference-driven granular structure generated by the wave nature of ultralight bosons. Since these fluctu…

astro-ph.GA2026

Equilibrium Core and Vortex Solutions of Bose Einstein Condensate Dark Matter around a Black Hole

Ivan Alvarez-Rios, Francisco S. Guzman

We present the construction of stationary solutions of Bose-Einstein condensate dark matter (BECDM) around a point-like gravitational source representing a black hole. The problem…

astro-ph.CO2025

Fermion-Boson Stars as Attractors in Fuzzy Dark Matter and Ideal Gas Dynamics

Ivan Alvarez-Rios, Francisco S. Guzman, Jens Niemeyer

In the context of Fuzzy Dark Matter (FDM) we study the core formation in the presence of an Ideal Gas (IG). Our analysis is based on the solution of the Schrödinger-Poisson-Euler…

astro-ph.GA2025

Black Holes as Condensation Points of Fuzzy Dark Matter Cores

Curicaveri Palomares-Chavez, Ivan Alvarez-Rios, Francisco S. Guzman

We simulate the formation of Fuzzy Dark Matter (FDM) cores in the presence of a Black Hole (BH) to explore whether BHs can serve as seeds for FDM core condensation. Our analysis is…

astro-ph.GA2025

Construction of ground state solutions of the Gross-Pitaevskii-Poisson system using genetic algorithms

Carlos Tena-Contreras, Ivan Alvarez-Rios, F. S. Guzman

We present the construction of the ground state of the Gross-Pitaevskii-Poisson equations using genetic algorithms. By employing numerical solutions, we develop an empirical formul…

astro-ph.GA2025

Unveiling Orbital Chaos: The Wild Heart of Fuzzy Dark Matter Structures

Ivan Alvarez-Rios, Francisco S. Guzman

In this paper we study the behavior of test particles on top of a galactic-type of Fuzzy Dark Matter (FDM) structure, characterized by the core-halo density profile found in simula…