activity
20142026
most citedTimelike geodesics of a modified gravity black hole immersed in an axially symmetric magnetic field

94 citations · 402 across the 16 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

11 papers · 1 filter

astro-ph.HE2026

High-energy Neutrino and Gamma Ray Emission from Clusters-like Perseus

Saqib Hussain, Gabrijela Zaharijas, Klaus Dolag

We calculate the high-energy gamma-ray and neutrino emissions from galaxy clusters like Perseus that host active galactic nuclei (AGNs). Our primary objective is to distinguish the…

astro-ph.HE2026

High-energy Multi-messenger Emission from Galaxy Clusters in the Local Universe

Saqib Hussain, Gabrijela Zaharijas, Klaus Dolag

The origin of diffuse neutrinos and -rays is unknown, and galaxy clusters hosting AGN and starburst galaxies are the most probable sources of these cosmic messengers. In this wo…

astro-ph.HE2023

Chasing Gravitational Waves with the Cherenkov Telescope Array

Jarred Gershon Green, Alessandro Carosi, Lara Nava +563

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts…

astro-ph.HE2023

Variability studies of active galactic nuclei from the long-term monitoring program with the Cherenkov Telescope Array

Guillaume Grolleron, Josefa Becerra González, Jonathan Biteau +13

Blazars are active galactic nuclei (AGN) with a relativistic jet oriented toward the observer. This jet is composed of accelerated particles which can display emission over the ent…

astro-ph.HE2023

Dark matter searches in dwarf spheroidal galaxies with the Cherenkov Telescope Array

Francesco Gabriele Saturni, Michele Doro, Aldo Morselli +1

Dark matter (DM) is one of the major components in the Universe. However, at present its existence is still only inferred through indirect astronomical observations. DM particles c…

astro-ph.HE2023

Neutrinos and gamma-rays from Galaxy Clusters constrained by the upper limits of IceCube

Saqib Hussain, Elisabete M. de Gouveia Dal Pino, Giulia Pagliaroli

Clusters of galaxies possess the capability to accelerate cosmic rays (CRs) to very high energy up to ~eV due to their large size and magnetic field strength which fav…

astro-ph.HE2023★ 1 cited

High-Energy Neutrino and Gamma Ray Production in Clusters of Galaxies

Saqib Hussain, Giulia Pagliaroli, Elisabete M. de Gouveia Dal Pino

We compute the contribution from clusters of galaxies to the diffuse neutrino and ray background. Due to their unique magnetic-field configuration, cosmic rays (CRs) with energ…

astro-ph.HE2022★ 18 cited

The Diffuse Gamma-Ray Flux from Clusters of Galaxies

Saqib Hussain, Rafael Alves Batista, Elisabete M. de Gouveia Dal Pino +1

The origin of the diffuse gamma-ray background (DGRB), the one that remains after subtracting all individual sources from observed gamma-ray sky, is unknown. The DGRB possibly enco…

astro-ph.HE2021

High-Energy Neutrino Production in Clusters of Galaxies

Saqib Hussain, Rafael Alves Batista, Elisabete de Gouveia Dal Pino +1

In this work, we compute the contribution from clusters of galaxies to the diffuse neutrino background. Clusters of galaxies can potentially produce cosmic rays (CRs) up to very-hi…

astro-ph.HE2021

High-Energy Neutrino Production in Clusters of Galaxies

Saqib Hussain, Rafael Alves Batista, Elisabete M. de Gouveia Dal Pino +1

Clusters of galaxies can potentially produce cosmic rays (CRs) up to very-high energies via large-scale shocks and turbulent acceleration. Due to their unique magnetic-field config…

astro-ph.HE2018★ 7 cited

Cosmic-ray propagation in the turbulent intergalactic medium

R. Alves Batista, E. M. de Gouveia Dal Pino, K. Dolag +1

Cosmic rays (CRs) may be used to infer properties of intervening cosmic magnetic fields. Conversely, understanding the effects of magnetic fields on the propagation of high-energy…