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

Fingerprint

gamma ray bursts
neutrinos
cosmic rays
predictions
energy
galactic clusters
afterglows
active galactic nuclei
flares
galaxies
detectors

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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
Murase, Kohta. / High-energy neutrinos and gamma-ray bursts. KEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe - Interplay between High Energy Physics and Cosmophysics. Vol. 1040 2008. pp. 170-174
@inproceedings{48a2fc032f4944c284b8638d2cf12768,
title = "High-energy neutrinos and gamma-ray bursts",
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.",
author = "Kohta Murase",
year = "2008",
month = "9",
day = "26",
doi = "10.1063/1.2981541",
language = "English (US)",
isbn = "9780735405677",
volume = "1040",
pages = "170--174",
booktitle = "KEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe - Interplay between High Energy Physics and Cosmophysics",

}

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, KEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe, AIU 2008, Tsukuba, Japan, 3/12/08. https://doi.org/10.1063/1.2981541

High-energy neutrinos and gamma-ray bursts. / Murase, Kohta.

KEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe - Interplay between High Energy Physics and Cosmophysics. Vol. 1040 2008. p. 170-174.

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

TY - GEN

T1 - High-energy neutrinos and gamma-ray bursts

AU - Murase, Kohta

PY - 2008/9/26

Y1 - 2008/9/26

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=52249104015&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=52249104015&partnerID=8YFLogxK

U2 - 10.1063/1.2981541

DO - 10.1063/1.2981541

M3 - Conference contribution

SN - 9780735405677

VL - 1040

SP - 170

EP - 174

BT - KEK Cosmophysics Group Inaugural Conference - Accelerators in the Universe - Interplay between High Energy Physics and Cosmophysics

ER -

Murase K. 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. 2008. p. 170-174 https://doi.org/10.1063/1.2981541