activity
20052026
most citedOn the core-halo distribution of dark matter in galaxies

112 citations · 3k across the 133 of their papers we have counts for

collaborators

137 papers

gr-qc2026

Charging of rotating black holes: kinetic simulations of black hole magnetospheres

Martin Kološ, Farukh Abdulkhamidov, Arman Tursunov +2

Whether a rotating black hole (BH) immersed in an external magnetic field charges up to the Wald value , where and are the BH mass and spin parameter, and $…

astro-ph.HE2026

GRB 220101A: a most energetic erg long GRB triggered by two supernovae 3.5 seconds apart

R. Ruffini, Y. Aimuratov, L. M. Becerra +10

GRB 220101A is a long GRB, with a total energy exceeding erg with a redshift and one of the largest ever high-quality multi-wavelength observational coverage,…

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*…

astro-ph.HE2024★ 1 cited

X-ray pulsed light curves of highly compact neutron stars as probes of scalar-tensor theories of gravity

Tulio Ottoni, Jaziel G. Coelho, Rafael C. R. de Lima +2

The strong gravitational potential of neutron stars (NSs) makes them ideal astrophysical objects for testing extreme gravity phenomena. We explore the potential of NS X-ray pulsed…

astro-ph.GA2024

Fermionic Dark Matter spikes: origin and growth of Black Hole seeds

Valentina Crespi, Carlos R. Argüelles, Jorge A. Rueda

We characterize the overdensity (spike) of fermionic dark matter (DM) particles around a supermassive black hole (SMBH) within a general relativistic analysis. The initial DM halo…

astro-ph.HE2024★ 2 cited

Ten Supernova-rise in Binary Driven Gamma-ray Bursts

R. Ruffini, C. L. Bianco, Liang Li +6

The observation of a gamma-ray burst (GRB) associated with a supernova (SN) coincides remarkably with the energy output from a binary system comprising a very massive carbon-oxygen…