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Št. zadetkov: 4
Izvirni znanstveni članek
Oznake: pulsar wind nebulae;neutrinos;gamma-rays;multimessenger astronomy;
In this work, we provide a phenomenological description of the population of galactic TeV pulsar wind nebulae (PWNe) based on suitable assumptions for their space and luminosity distribution. We constrain the general features of this population by assuming that it accounts for the majority of bright ...
Leto: 2023 Vir: Repozitorij Univerze v Novi Gorici (RUNG)
Objavljeni znanstveni prispevek na konferenci
Oznake: multimessenger astronomy;pulsar wind nebulae;gamma rays;neutrinos;
In the hypothesis that the majority of bright TeV sources detected by H.E.S.S. are powered by pulsar activity, like, e.g., pulsar wind nebulae (PWN) or TeV halos, we estimate the main properties of the Galactic pulsar population. We obtain constraints on the spin-down time τsd, the initial period P0 ...
Leto: 2024 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)
Objavljeni znanstveni prispevek na konferenci
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)
Št. zadetkov: 4
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