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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THE COLLIMATION AND ENERGETICS OF THE BRIGHTESTSWIFTGAMMA-RAY BURSTS
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Energetics and Luminosity Function of Gamma‐Ray Bursts
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Self-citationMagnetohydrodynamic simulations of gamma-ray burst jets: Beyond the progenitor star
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GRB 021004: Reverse Shock Emission
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Self-citationDai, Z.-G., & Cheng, K. S. (2001) · The Astrophysical Journal · doi:10.1086/323566 · Cited by 147
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Self-citationImplications of the early X-ray afterglow light curves of Swift gamma-ray bursts
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An Unexpectedly Swift Rise in the Gamma-Ray Burst Rate
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Steepening of Afterglow Decay for Jets Interacting with Stratified Media
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Self-citationImpulsive acceleration of strongly magnetized relativistic flows
Granot, J., Komissarov, S. S., & Spitkovsky, A. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17770.x · Cited by 144
How gravitational-wave observations can shape the gamma-ray burst paradigm
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THE METAL AVERSION OF LONG-DURATION GAMMA-RAY BURSTS
Graham, J. F., & Fruchter, A. S. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/774/2/119 · Cited by 139
Goldreich, P., & Julian, W. H. (1970) · The Astrophysical Journal · doi:10.1086/150486 · Cited by 139
A Simple Type of Magnetically Driven Jets: an Astrophysical Plasma Gun
Contopoulos, J. (1995) · The Astrophysical Journal · doi:10.1086/176170 · Cited by 138
The effective acceleration of plasma outflow in the paraboloidal magnetic field
Beskin, V. S., & Nokhrina, E. E. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.09957.x · Cited by 135
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Self-citationSmooth light curves from a bumpy ride: relativistic blast wave encounters a density jump
Ehud Nakar, A., & Granot, J. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12245.x · Cited by 135
McKinney, J. C., & Narayan, R. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.11301.x · Cited by 135
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Curvature Effects in Gamma‐Ray Burst Colliding Shells
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Discovery of Early Optical Emission from GRB 021211
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Constraining the Structure of Gamma‐Ray Burst Jets through the Afterglow Light Curves
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Self-citationRebrightening of XRF 030723: Further Evidence for a Two‐Component Jet in a Gamma‐Ray Burst
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Relativistic Wind Bubbles and Afterglow Signatures
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Self-citationLORENTZ-FACTOR–ISOTROPIC-LUMINOSITY/ENERGY CORRELATIONS OF GAMMA-RAY BURSTS AND THEIR INTERPRETATION
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Gravitational Radiation from Gamma‐Ray Burst Progenitors
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Two‐Component Jet Models of Gamma‐Ray Burst Sources
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Short-living Supermassive Magnetar Model for the Early X-ray Flares Following Short GRBs
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Power Density Spectra of Gamma-Ray Bursts in the Internal Shock Model
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Dynamical Evolution, Light Curves, and Spectra of Spherical and Collimated Gamma‐Ray Burst Remnants
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Self-citationCorrelations of Prompt and Afterglow Emission inSwiftLong and Short Gamma‐Ray Bursts
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Self-citationThe redshift and afterglow of the extremely energetic gamma-ray burst GRB 080916C
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Particle Transport in Tangled Magnetic Fields and Fermi Acceleration at Relativistic Shocks
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Self-citationWinds from massive stars: implications for the afterglows of -ray bursts
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Self-citationDeceleration of arbitrarily magnetized GRB ejecta: the complete evolution
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Nagakura, H., Ito, H., Kiuchi, K., & Yamada, S. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/731/2/80 · Cited by 110
Discovery of an Afterglow Extension of the Prompt Phase of Two Gamma-Ray Bursts Observed by Swift
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Self-citationAfterglows, Redshifts, and Properties ofSwiftGamma‐Ray Bursts
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Opacity Buildup in Impulsive Relativistic Sources
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Self-citationGRB 061121: Broadband Spectral Evolution through the Prompt and Afterglow Phases of a Bright Burst
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The Afterglow of GRB 990123 and a Dense Medium
戴子高, & Lu, T. (1999) · The Astrophysical Journal · doi:10.1086/312127 · Cited by 106
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A NEW CLASSIFICATION METHOD FOR GAMMA-RAY BURSTS
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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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