Neutrinos from Supernovae

Irene Tamborra; Kohta Murase

doi:10.1007/s11214-018-0468-7

Neutrinos from Supernovae

2 Citations (Scopus)

Abstract

Neutrinos are fundamental particles in the collapse of massive stars. Because of their weakly interacting nature, neutrinos can travel undisturbed through the stellar core and be direct probes of the still uncertain and fascinating supernova mechanism. Intriguing recent developments on the role of neutrinos during the stellar collapse are reviewed, as well as our current understanding of the flavor conversions in the stellar envelope. The detection perspectives of the next burst and of the diffuse supernova background will be also outlined. High-energy neutrinos in the GeV-PeV range can follow the MeV neutrino emission. Various scenarios concerning the production of high-energy neutrinos are discussed.

Original language	English
Article number	31
Journal	Space Science Reviews
Volume	214
Issue number	1
Number of pages	21
ISSN	0038-6308
DOIs	https://doi.org/10.1007/s11214-018-0468-7
Publication status	Published - 1 Feb 2018

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title = "Neutrinos from Supernovae",

abstract = "Neutrinos are fundamental particles in the collapse of massive stars. Because of their weakly interacting nature, neutrinos can travel undisturbed through the stellar core and be direct probes of the still uncertain and fascinating supernova mechanism. Intriguing recent developments on the role of neutrinos during the stellar collapse are reviewed, as well as our current understanding of the flavor conversions in the stellar envelope. The detection perspectives of the next burst and of the diffuse supernova background will be also outlined. High-energy neutrinos in the GeV-PeV range can follow the MeV neutrino emission. Various scenarios concerning the production of high-energy neutrinos are discussed.",

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Neutrinos from Supernovae

Abstract

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