activity
20062026
most citedMulti-state Boson Stars

113 citations · 1.1k across the 31 of their papers we have counts for

collaborators

32 papers

gr-qc2026

Gravitational confinement of ghost scalar fields in neutron stars

Argelia Bernal, Víctor Jaramillo, Néstor A. Montiel-Hernández +2

We investigate the effects, stability, and nonlinear dynamics of ghost scalar matter modeled as a field with a negative kinetic term confined within the cores of neutron stars. To…

gr-qc2025★ 1 cited

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-ph2025

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…

gr-qc2024★ 5 cited

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.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…

astro-ph.GA2023

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…