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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

Gamma-ray bursts and the fireball model

TL;DR: In this article, it was shown that the inner engine that accelerates the relativistic flow is hidden from direct observations and therefore it is difficult to infer its structure directly from current observations.
Journal ArticleDOI

Unsteady outflow models for cosmological gamma-ray bursts

TL;DR: In this paper, the authors proposed a mechanism for cosmological bursts that requires less extreme assumptions (in respect of Gamma-values, freedom from baryonic contamination, etc.) than earlier proposals.
Journal ArticleDOI

Gamma-ray bursts as the death throes of massive binary stars

TL;DR: In this article, it was shown that gamma-ray bursts are created in the mergers of double neutron star binaries and black hole neutron star binary at cosmological distances, and the strongest bursts should be found close to, but not at the centers of, galaxies at redshifts of order 0.1, and should be accompanied by bursts of gravitational radiation from the spiraling-in binary which could be detected by LIGO.
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Optical and long wavelength afterglow from gamma-ray bursts

TL;DR: In this article, the authors discuss the evolution of cosmological gamma-ray burst remnants, consisting of the cooling and expanding fireball ejecta together with any swept-up external matter.
Journal ArticleDOI

Fluid dynamics of relativistic blast waves

TL;DR: In this paper, a fluid dynamical treatment of an ultra-relativistic spherical blast wave enclosed by a strong shock is presented, and a simple similarity solution describing the explosion of a fixed amount of energy in a uniform medium is derived, and generalized to include cases in which power is supplied by a central source and the density of the external medium varies with radius.
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