activity
20242026
collaborators

6 papers

gr-qc2026

Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number

Miguel Alcubierre, Juan Barranco, Argelia Bernal +5

We present new spherically symmetric solutions of the Einstein-Klein-Gordon equations in a quasi-stationary approximation that describe self-gravitating scalar field configurations…

hep-ph2026

Probing a minimal dark gauge sector via microlensing of compact dark objects

Juan Barranco, Argelia Bernal, Víctor Jaramillo +2

We introduce a minimal Dark Standard Model (DSM) consisting of a single spin-0 particle with dark gauge symmetry, and completely decoupled from the visible sector. Character…

astro-ph.CO2026

Dark-to-black super accretion as a mechanism for early supermassive black hole growth

Nicolas Sanchis-Gual, Juan Barranco, Juan Carlos Degollado +1

The discovery of supermassive black holes with masses at redshifts challenges conventional formation scenarios based on baryonic accretion and…

gr-qc2025

Gravitational atoms beyond the test field limit: The case of Sgr A* and ultralight dark matter

Miguel Alcubierre, Juan Barranco, Argelia Bernal +5

We construct gravitational atoms including self-gravity, obtaining solutions of the Einstein-Klein-Gordon equations for a scalar field surrounding a non-rotating black hole in a qu…

astro-ph.GA2025

Thermodynamics sheds light on the nature of dark matter galactic halos

Andrés Aceña, Juan Barranco, Argelia Bernal +1

In spherical symmetry, the gravitational potential is uniquely determined by the rotational velocity profile. Numerous galaxies exhibit a universal velocity profile from which a un…

astro-ph.HE2024

Constrains on dark matter cross section with standard model particles from the orbital period decay of binary pulsars

Gonzalo Agustin Lucero, Argelia Bernal, Juan Barranco +1

It is shown that the data from the orbital period decay of binary pulsars give strong constraints on the dark matter-nucleons cross section. The limits are robust and competitive b…