High-energy neutrinos and gamma-ray bursts

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

High-energy neutrinos from gamma-ray bursts (GRBs) have been expected in various scenarios. Many predictions for the prompt and afterglow emission were done in the pre-Swift era. After the launch of Swift, several new discoveries such as flares have allowed us to expect additional possibilities of the neutrino emission from GRBs. In this paper, we overview predictions of the high-energy neutrino emission from GRBs, and compare them with several predictions for other sources such as active galactic nuclei (AGN) and clusters of galaxies. High-energy neutrino signals may be detected by future-coming large neutrino detectors such as IceCube and KM3Net. If detected, they should be very useful for knowing the nature of cosmic-ray acceleration sites. It also helps us to reveal the possible connection between ultra-high-energy cosmic rays (UHECRs) and GRBs.

Original languageEnglish (US)
Title of host publicationKEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe - Interplay between High Energy Physics and Cosmophysics
Pages170-174
Number of pages5
Volume1040
DOIs
StatePublished - Sep 26 2008
EventKEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe, AIU 2008 - Tsukuba, Japan
Duration: Mar 12 2008Mar 14 2008

Other

OtherKEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe, AIU 2008
CountryJapan
CityTsukuba
Period3/12/083/14/08

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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  • Cite this

    Murase, K. (2008). High-energy neutrinos and gamma-ray bursts. In KEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe - Interplay between High Energy Physics and Cosmophysics (Vol. 1040, pp. 170-174) https://doi.org/10.1063/1.2981541