95 citations · 517 across the 33 of their papers we have counts for
34 papers
Ultra-high-energy cosmic ray acceleration by magnetic reconnection in relativistic jets and the origin of very high energy emission
E. De Gouveia Dal Pino, T. E. Medina-Torrejon, L. H. S. Kadowaki +2
Relativistic jets are believed to be born magnetically dominated. Very and ultra-high energy cosmic rays can be efficiently accelerated by magnetic reconnection in these sources. W…
Gamma-ray Emission Properties of Four Bright Fermi-LAT AGNs: Implications on Emission Processes
Pankaj Kushwaha, Atreyee Sinha, Ranjeev Misra +2
The X-ray, Ultraviolet, Optical emission from radio-quiet AGNs, black hole binaries, and other compact sources, in general, follow a lognormal flux distribution, a linear rms-flux…
The Cherenkov Telescope Array view of the Galactic Center region
Aion Viana, Sofia Ventura, Daniele Gaggero +22
Among all the high-energy environments of our Galaxy, the Galactic Center (GC) region is definitely the richest. It harbors a large amount of non-thermal emitters, including the cl…
A statistical study of fast magnetic reconnection in turbulent accretion disks and jets
Luís H. S. Kadowaki, Elisabete M. de Gouveia Dal Pino, Tania E. Medina-Torrejón
Fast magnetic reconnection events can play an important role in accretion disk systems. A potential model to explain the non-thermal very-high-energy (VHE) emission (from GeV to Te…
Magnetic Reconnection, Cosmic Ray Acceleration, and Gamma-Ray emission around Black Holes and Relativistic Jets
Elisabete M. de Gouveia Dal Pino, Rafael Alves Batista, Grzergorz Kowal +2
Particle acceleration by magnetic reconnection is now recognized as an important process in magnetically dominated regions of galactic and extragalactic black hole sources. This pr…
Numerical models of neutrino and gamma-ray emission from magnetic reconnection in the core of radio-galaxies
Juan Carlos Rodríguez-Ramírez, Elisabete Maria de Gouveia Dal Pino, Rafael Alves Batista
Non-blazar radio-galaxies emitting in the very-high-energy (VHE; >100 GeV) regime offer a unique perspective for probing particle acceleration and emission processes in black hole…