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Open AccessJournal ArticleDOI

Gamma-ray bursts – a puzzle being resolved ☆

Tsvi Piran, +1 more
- 01 Aug 2000 - 
- Vol. 333, pp 529-553
TLDR
The recent discovery of GRB afterglow has demonstrated that we are on the right track towards the resolution of this long standing puzzle as discussed by the authors, and the current understanding implies that GRBs signal the birth of stellar mass black holes.
About
This article is published in Physics Reports.The article was published on 2000-08-01 and is currently open access. It has received 207 citations till now. The article focuses on the topics: Gamma-ray burst & Gamma-ray burst progenitors.

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Citations
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Journal ArticleDOI

The physics of gamma-ray bursts

TL;DR: A review of the current theoretical understanding of the physical processes believed to take place in GRB's can be found in this article, where the authors focus on the afterglow itself, the jet break in the light curve, and the optical flash that accompanies the GRB.
Journal ArticleDOI

Beaming in gamma-ray bursts: evidence for a standard energy reservoir

TL;DR: In this article, a comprehensive sample of all gamma-ray burst (GRB) afterglows with known distances is presented, and their conical opening angles are derived based on observed broadband breaks in their light curves.
Journal ArticleDOI

The physics of gamma-ray bursts & relativistic jets

TL;DR: 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, can be found in this paper.
Journal ArticleDOI

The Physics of Gamma-Ray Bursts and Relativistic Jets

TL;DR: A comprehensive review of major developments in the understanding of gamma-ray bursts can be found in this article, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered.
Journal ArticleDOI

Accretion Models of Gamma‐Ray Bursts

TL;DR: In this article, it was shown that if the viscosity parameter a in the NDAF has a standard value of D0.1, these models can explain short gamma-ray bursts with durations under a second, but they are unlikely to produce long GRBs with tens or hundred of seconds.
References
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Journal ArticleDOI

Images and spectra from the interior of a relativistic fireball

TL;DR: In this paper, the spectrum and the light curve of an adiabatic blast wave were derived from the Blandford-McKee self-similar solution, showing that the expected light curve and spectra are flat near the peak.
Journal ArticleDOI

Evolution of Binary Compact Objects That Merge

TL;DR: In this article, the authors calculated the mass of the first neutron star to be 2.4 M and showed that if the two massive binaries are sufficiently close in mass, not more than 5% apart, then their common hydrogen envelope is expelled by the tightening in the double He star system, with attendant hydrodynamical coupling to the envelope.
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Radio Transients from Gamma-Ray Bursters

TL;DR: In this paper, the authors estimate that the strongest gamma-ray bursts may be followed by radio transients with peak fluxes as high as 20 mJy, depending on the distance scale.
Journal ArticleDOI

Neutrino bursts from gamma-ray bursts

TL;DR: In this article, it was shown that neutrino bursts are the likely consequence of the highly super-Eddington luminosity of the sources, and the strongest gamma-ray bursts are observed to deliver approximately 10(exp -4) ergs/sq cm in 100-200 keV photons.
Journal ArticleDOI

Cooling Time Scales and Temporal Structure of Gamma-Ray Bursts

TL;DR: In this paper, the authors estimate the cooling time scale of the shocked regions for electrons of various Lorentz factors, focusing in particular on those electrons whose radiation falls within the energy detection range of the BATSE detectors.
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