Particle Astrophysics with High and Ultrahigh Energy Neutrinos

Fuente: arXiv
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Autores principales: Fang, Ke, Murase, Kohta
Formato: Preprint
Publicado: 2025
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author Fang, Ke
Murase, Kohta
author_facet Fang, Ke
Murase, Kohta
contents We summarize recent results of the observations of high (1 TeV-100 PeV) and ultrahigh ($\geq 100$ PeV) energy neutrinos, including the detection of a diffuse cosmic high-energy neutrino background, the identification of the first neutrino source candidates, and the observation of high-energy neutrinos from the Galactic plane. These findings open a new window to the universe by enabling the use of neutrinos to probe the cosmos that are otherwise inaccessible via photons. Although the origins of most detected neutrinos remain uncertain, we highlight several distinctive features of their sources that have emerged from current observations.
format Preprint
id arxiv_https___arxiv_org_abs_2512_00660
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Particle Astrophysics with High and Ultrahigh Energy Neutrinos
Fang, Ke
Murase, Kohta
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
We summarize recent results of the observations of high (1 TeV-100 PeV) and ultrahigh ($\geq 100$ PeV) energy neutrinos, including the detection of a diffuse cosmic high-energy neutrino background, the identification of the first neutrino source candidates, and the observation of high-energy neutrinos from the Galactic plane. These findings open a new window to the universe by enabling the use of neutrinos to probe the cosmos that are otherwise inaccessible via photons. Although the origins of most detected neutrinos remain uncertain, we highlight several distinctive features of their sources that have emerged from current observations.
title Particle Astrophysics with High and Ultrahigh Energy Neutrinos
topic High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2512.00660