The DOI matches its Crossref record; 527 of the 527 references it cites were found in a registry or an index.
The physics of gamma-ray bursts & relativistic jets
Open accessAbstract
Abstract We provide a comprehensive review of major developments in our understanding of gamma-ray bursts, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered. We describe the observational properties of photons from the radio to 100s GeV bands, both in the prompt emission and the afterglow phases. Mechanisms for the generation of these photons in GRBs are discussed and confronted with observations to shed light on the physical properties of these explosions, their progenitor stars and the surrounding medium. After presenting observational evidence that a powerful, collimated, jet moving at close to the speed of light is produced in these explosions, we describe our current understanding regarding the generation, acceleration, and dissipation of the jet. We discuss mounting observational evidence that long duration GRBs are produced when massive stars die, and that at least some short duration bursts are associated with old, roughly solar mass, compact stars. The question of whether a black-hole or a strongly magnetized, rapidly rotating neutron star is produced in these explosions is also discussed. We provide a brief summary of what we have learned about relativistic collisionless shocks and particle acceleration from GRB afterglow studies, and discuss the current understanding of radiation mechanism during the prompt emission phase. We discuss theoretical predictions of possible high-energy neutrino emission from GRBs and the current observational constraints. Finally, we discuss how these explosions may be used to study cosmology, e.g. star formation, metal enrichment, reionization history, as well as the formation of first stars and galaxies in the universe.
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Self-citationON THE HIGH-ENERGY EMISSION OF THE SHORT GRB 090510
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Self-citationProduction of Magnetic Energy by Macroscopic Turbulence in GRB Afterglows
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Self-citationAFTERGLOW OF A BINARY NEUTRON STAR MERGER
Shibata, M., Suwa, Y., Kiuchi, K., & Ioka, K. (2011) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/734/2/l36 · Cited by 60
The Swift/FermiGRB 080928 from 1 eV to 150 keV
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The interpretation and implication of the afterglow of GRB 060218
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New three-parameter correlation for gamma-ray bursts with a plateau phase in the afterglow
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Thick Fireballs and the Steep Decay in the Early X‐Ray Afterglow of Gamma‐Ray Bursts
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MODELING THE BROADBAND EMISSION OF GRB 090902B
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Is GeV emission from Gamma-Ray Bursts of external shock origin?
Maxham, A., Zhang, B.-B., & Zhang, B. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.18648.x · Cited by 56
Self-citationPrompt optical emission and synchrotron self-absorption constraints on emission site of GRBs
Shen, R.-F., & Zhang, B. (2009) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2009.15212.x · Cited by 56
Self-citationThe dynamics of a highly magnetized jet propagating inside a star
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Self-citationProbing the nature of high-z short GRB 090426 with its early optical and X-ray afterglows
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The Spectral Lag of GRB 060505: A Likely Member of the Long-Duration Class
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Self-citationCOLLAPSAR ACCRETION AND THE GAMMA-RAY BURST X-RAY LIGHT CURVE
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Self-citationThe nature of H i absorbers in gamma-ray burst afterglows: clues from hydrodynamic simulations
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Self-citationGRB 110721A: PHOTOSPHERE “DEATH LINE” AND THE PHYSICAL ORIGIN OF THE GRB BAND FUNCTION
Zhang, B., Lu, R.-J., Liang, E.-W., & Wu, X.-F. (2012) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/758/2/l34 · Cited by 46
Self-citationAN OBSERVED CORRELATION BETWEEN THERMAL AND NON-THERMAL EMISSION IN GAMMA-RAY BURSTS
Burgess, J. M., Preece, R. D., Ryde, F., Veres, P., Mészáros, P., Connaughton, V., Briggs, M., Pe'er, A., Iyyani, S., Goldstein, A., et al. (2014) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/784/2/l43 · Cited by 45
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Self-citationSwiftDiscovery of Gamma‐Ray Bursts without a Jet Break Feature in Their X‐Ray Afterglows
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Gamma-ray bursts: polarization of afterglows from two-component jets
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GRB 070125: The First Long‐Duration Gamma‐Ray Burst in a Halo Environment
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-ray burst internal shocks with magnetization
Fan, Y.-Z., Wei, D. M., & Zhang, B. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08263.x · Cited by 43
Self-citationThe Ionizing Efficiency of the First Stars
Venkatesan, A., & Truran, J. W. (2003) · The Astrophysical Journal · doi:10.1086/378399 · Cited by 41
Multicolor Shallow Decay and Chromatic Breaks in the GRB 050319 Optical Afterglow
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Metadata
- Authors
- Kumar, P., & Zhang, B.
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2015-02
- Volume
- 561
- Pages
- 1-109
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W2141952413
- Cited by
- 952
- References
- 527
- FWCI
- 33.28
- Type
- journal article
- Language
- en
- Open access
- green
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Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
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Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.