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From the 1 of 10 linked papers with an AI index.

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20242026
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10 papers

astro-ph.SR2026

Magnetic Reconnection Process in Partially Ionized Fluids: Insights from the Solar Chromosphere

Adrian R. Montañez-Lobo, Fabio D. Lora-Clavijo

The paper studies how magnetic reconnection operates in the partially ionized solar chromosphere, using 2.5D two‑fluid MHD simulations that include elastic and inelastic collisions…

astro-ph.HE2026

Relativistic Common-envelope Dynamics of a Stellar-mass Black Hole II: Kerr Black Hole

Alejandro Cruz-Osorio, Fabio D. Lora-Clavijo

The common envelope phase plays a critical role in binary system evolution. In this study, we investigate the mass and momentum accretion rates during the interaction between a ste…

gr-qc2026

Nonradial oscillations of realistic anisotropic neutron stars: Axial modes

Jose F. Rodriguez-Ruiz, L. M. Becerra, F. D. Lora-Clavijo

Non-radial oscillation modes of neutron stars serve as diagnostics of their internal composition and relativistic structure. In this work, we investigate the perturbations of stati…

gr-qc2025

On the Stability of Anisotropic Neutron Stars

L. M. Becerra, E. A. Becerra-Vergara, F. D. Lora-Clavijo +1

We model anisotropic neutron stars using three distinct prescriptions for pressure anisotropy, the Horvat, Bowers-Liang, and Covariant models, and three equations of state with dif…

astro-ph.HE2025

Rotating neutron stars: anisotropy model comparison

L. M. Becerra, E. A. Becerra-Vergara, F. D. Lora-Clavijo

We build slowly rotating anisotropic neutron stars using the Hartle-Thorne formalism, employing three distinct anisotropy models--Horvat, Bowers-Liang, and a covariant model--to ch…

gr-qc2025

Shadow and gravitational lensing produced by the nonlinear accretion of a scalar field onto a black hole

J. C. Acevedo-Muñoz, F. D. Lora-Clavijo, A. Cruz-Osorio

The hypothesis that classical scalar fields could constitute dark matter on galactic and cosmic scales has garnered significant interest. In scenarios where supermassive black hole…