GeV-TeV emission from γ-ray bursts

P. Mészáros; S. Razzaque; B. Zhang

doi:10.1016/j.newar.2003.12.022

GeV-TeV emission from γ-ray bursts

P. Mészáros
, S. Razzaque
, B. Zhang

Research output: Contribution to journal › Short survey › peer-review

7 Scopus citations

Abstract

Most of the current knowledge about γ-ray bursts (GRB) is based on electromagnetic observations at MeV and lower energies. Here, we focus on some recent theoretical work on GRB, in particular the higher energy (GeV-TeV) photon emission, and the expected TeV and higher energy neutrino emission.

Original language	English (US)
Pages (from-to)	445-451
Number of pages	7
Journal	New Astronomy Reviews
Volume	48
Issue number	5-6
DOIs	https://doi.org/10.1016/j.newar.2003.12.022
State	Published - Apr 2004

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1016/j.newar.2003.12.022

Cite this

@article{cfa8602fa50d415c8c17849b51f8d590,

title = "GeV-TeV emission from γ-ray bursts",

abstract = "Most of the current knowledge about γ-ray bursts (GRB) is based on electromagnetic observations at MeV and lower energies. Here, we focus on some recent theoretical work on GRB, in particular the higher energy (GeV-TeV) photon emission, and the expected TeV and higher energy neutrino emission.",

author = "P. M{\'e}sz{\'a}ros and S. Razzaque and B. Zhang",

note = "Funding Information: This research has been partially supported through NASA NAG5-9192 and NSF AST-0098416.",

year = "2004",

month = apr,

doi = "10.1016/j.newar.2003.12.022",

language = "English (US)",

volume = "48",

pages = "445--451",

journal = "New Astronomy Reviews",

issn = "1387-6473",

publisher = "Elsevier B.V.",

number = "5-6",

}

TY - JOUR

T1 - GeV-TeV emission from γ-ray bursts

AU - Mészáros, P.

AU - Razzaque, S.

AU - Zhang, B.

N1 - Funding Information: This research has been partially supported through NASA NAG5-9192 and NSF AST-0098416.

PY - 2004/4

Y1 - 2004/4

N2 - Most of the current knowledge about γ-ray bursts (GRB) is based on electromagnetic observations at MeV and lower energies. Here, we focus on some recent theoretical work on GRB, in particular the higher energy (GeV-TeV) photon emission, and the expected TeV and higher energy neutrino emission.

AB - Most of the current knowledge about γ-ray bursts (GRB) is based on electromagnetic observations at MeV and lower energies. Here, we focus on some recent theoretical work on GRB, in particular the higher energy (GeV-TeV) photon emission, and the expected TeV and higher energy neutrino emission.

UR - https://www.scopus.com/pages/publications/1542610066

UR - https://www.scopus.com/pages/publications/1542610066#tab=citedBy

U2 - 10.1016/j.newar.2003.12.022

DO - 10.1016/j.newar.2003.12.022

M3 - Short survey

AN - SCOPUS:1542610066

SN - 1387-6473

VL - 48

SP - 445

EP - 451

JO - New Astronomy Reviews

JF - New Astronomy Reviews

IS - 5-6

ER -

GeV-TeV emission from γ-ray bursts

Abstract

All Science Journal Classification (ASJC) codes

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