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…

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…

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…

hep-ph2025

Constraining ultra light fermionic dark matter with Milky-Way observations

J. Barranco, A. Bernal, D. Delepine

The equation of state for a degenerate gas of fermions at zero temperature in the non-relativistic case is a polytrope, i.e. . If dark matter is modeled b…

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…