activity
20242026
collaborators

22 papers

astro-ph.HE2026

A Four-Dimensional Gaussian Random Field Generator for Modeling Spatiotemporal Variability in Astrophysical Sources

Alejandro Cárdenas-Avendaño, Diego Rubiera-Garcia, Frederic H. Vincent

Semi-analytic models of black-hole movies require both an emitting flow prescription and a time-dependent source variability. Existing prescriptions are often limited to either equ…

gr-qc2026

Regular Black Holes in General Relativity from Nonlinear Electrodynamics with de Sitter Cores

A. A. Araújo Filho, Ednaldo L. B. Junior, José Tarciso S. S. Junior +6

We present new regular black hole solutions in general relativity (GR) within a static, spherically symmetric framework governed by a variable equation of state, following the appr…

gr-qc2026

Black bounce solutions in a realistic dark matter halo from M60*

Ednaldo L. B. Junior, José Tarciso S. S. Junior, Francisco S. N. Lobo +5

We formulate a Simpson-Visser black bounce solution embedded in a dark matter halo. The latter is modeled using an empirical density profile calibrated from observations of the ell…

gr-qc2026

Matter environments around black holes: geodesics, light rings, and ultracompact configurations

Dylan S. Fonseca, Caio F. B. Macedo, Mateus Malato Corrêa +1

Astrophysical black holes are invariably embedded in matter environments whose gravitational influence can alter key strong-field features of the spacetime. In this work, we invest…

gr-qc2026

Scalar-Electromagnetic Couplings as Source of Deformed Black Hole: From Shadows to Thermodynamic Topology

Ednaldo L. B. Junior, José Tarciso S. S. Junior, Francisco S. N. Lobo +5

We reconstruct a static and spherically symmetric black hole geometry originally proposed as an effective metric by identifying a consistent matter source derived from a fundamenta…

gr-qc2026

Observational appearance and photon rings of non-singular black holes from anisotropic fluids

David Díaz-Guerra, Angel Rincon, Diego Rubiera-Garcia

We consider the optical appearance of a non-singular, spherically symmetric black hole from Eddington-inspired Born-Infeld gravity coupled to anisotropic fluids. Such a black hole…