output
19972026
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations

336 papers

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…

hep-ex2026

Latin American HECAP Physics Briefing Book 2025

Mario A. Acero, Alexis A. Aguilar-Arevalo, Belén Andrada +24

The first process for the Latin American Strategy Forum for Research Infrastructure for High Energy, Cosmology and Astroparticle Physics (LASF4RI-HECAP) came to a conclusion in Oct…

cs.CV2026

Ozone Cues Mitigate Reflected Downwelling Radiance in LWIR Absorption-Based Ranging

Unay Dorken Gallastegi, Wentao Shangguan, Vaibhav Choudhary +4

Passive long-wave infrared (LWIR) absorption-based ranging relies on atmospheric absorption to estimate distances to objects from their emitted thermal radiation. First demonstrate…

astro-ph.HE2026

Search for ultra-high energy neutrons from Galactic sources with the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Abdul Halim, P. Abreu +357

Deflections in the propagation of charged ultra-high-energy cosmic rays (UHECRs) caused by magnetic fields make the identification of their sources challenging. On the other hand,…

gr-qc2026

Jacobson's thermodynamic approach to classical gravity applied to non-Riemannian geometries: remarks on the simplicity of Nature

Jhan N. Martinez, Jose F. Rodriguez-Ruiz, Yeinzon Rodriguez

Three decades ago, Ted Jacobson surprised us with a very appealing approach to classical gravity. According to him, the gravitational field equations are the consequence of the fir…

astro-ph.GA2025★ 1 cited

The dynamics of S-stars and G-sources orbiting a supermassive compact object made of fermionic dark matter

Valentina Crespi, Carlos R. Argüelles, Eduar A. Becerra-Vergara +4

Surrounding Sgr A*, a cluster of young and massive stars coexist with a population of dust-enshrouded objects, whose astrometric data can be used to scrutinize the nature of Sgr A*…