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Št. zadetkov: 7
Objavljeni znanstveni prispevek na konferenci
Oznake: Monte Carlo simulations;cosmic rays;intragalactic medium;
We present results of the propagation of high-energy cosmic rays (CRs) in the intracluster medium (ICM). To this end, we employ three-dimensional cosmological magnetohydrodynamical simulations of the turbulent intergalactic medium to explore the propagation of CRs with energies between 1e14 and 1e19 ...
Leto: 2019 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Izvirni znanstveni članek
Oznake: galaxy cluster;cosmic rays;gamma rays;neutrinos;
Clusters of galaxies possess the capability to accelerate cosmic rays (CRs) to very high energy up to ∼1018 eV due to their large size and magnetic field strength, which favor CR confinement for cosmological times. During their confinement, they can produce neutrinos and γ-rays out of interactions w ...
Leto: 2024 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
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Oznake: multimessenger astronomy;perseus cluster;gamma rays;neutrinos;cosmic rays;
We compute the contribution from clusters of galaxies to the diffuse neutrino and γ− ray background. Due to their unique magnetic-field configuration, cosmic rays (CRs) with energy ≤1e17 eV can be confined within these structures over cosmological time scales, and generate secondary particles, inc ...
Leto: 2024 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Izvirni znanstveni članek
Oznake: galaxy clusters;gamma-rays;neutrinos;
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 encompasses contributions from different source populations such as star-forming galaxies, starburst galaxies, active galact ...
Leto: 2023 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Izvirni znanstveni članek
Oznake: clusters of galaxies;AGN;neutrinos;gamma rays;cosmic rays;magnetic field;
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 configuration, CRs with energy ≤1017 eV can be trapped within these structures over cosmological time-scales, and generate sec ...
Leto: 2021 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Objavljeni znanstveni prispevek na konferenci
Oznake: astroparticle physics;galaxy clusters;gamma rays;neutrinos;cosmic rays;
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-high energies via large-scale shocks and turbulent acceleration. Due to their unique magnetic-field configuration, CRs wit ...
Leto: 2022 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Objavljeni znanstveni prispevek na konferenci
Oznake: cosmic rays;ICM;IGM;gamma rays;neutrinos;
We present results of the propagation of high-energy cosmic rays (CRs) and their secondaries in the intracluster medium (ICM). To this end, we employ three-dimensional cosmological magnetohydrodynamical simulations of the turbulent intergalactic medium to explore the propagation of CRs with energies ...
Leto: 2021 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Št. zadetkov: 7
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