activity
20122026
most citedOpen Questions in Cosmic-Ray Research at Ultrahigh Energies

195 citations · 293 across the 9 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

Simulating the LOcal Web (SLOW): VII. Intergalactic magnetic field models for multi-messenger applications

Johannes Stoiber, Klaus Dolag, Francesca Capel +4

Context. The propagation of ultra-high-energy cosmic rays (UHECRs) and ultra-high-energy gamma-rays remains an open question in astroparticle physics, with the intergalactic magnet…

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.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.HE2019★ 195 cited

Open Questions in Cosmic-Ray Research at Ultrahigh Energies

Rafael Alves Batista, Jonathan Biteau, Mauricio Bustamante +13

We review open questions and prospects for progress in ultrahigh-energy cosmic ray (UHECR) research, based on a series of discussions that took place during the `The High-Energy Un…

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…

astro-ph.CO2017★ 61 cited

Limiting Magnetic Fields in the Cosmic Web with Diffuse Radio Emission

S. Brown, T. Vernstrom, E. Carretti +7

We set limits on the presence of the synchrotron cosmic web through the cross-correlation of the 2.3 GHz S-PASS survey with a model of the local cosmic web derived from constrained…

astro-ph.CO2014★ 11 cited

Cluster Radio Halos at the crossroads between astrophysics and cosmology in the SKA era

R. Cassano, G. Bernardi, G. Brunetti +16

Giant Radio Halos (RH) are diffuse, Mpc-sized, synchrotron radio sources observed in a fraction of merging galaxy clusters. The current scenario for the origin of RHs assumes that…

astro-ph.HE2012★ 1 cited

A new Monte Carlo Generator for Ultra-High Energy Cosmic Rays from the Local and Distant Universe

Klaus Dolag, Martin Erdmann, Gero Müller +2

For the understanding of the origin and propagation of ultra-high energy cosmic rays (UHECR) we developed a new approach to simulating UHECRs from an arbitrary number of sources ba…