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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

Euclidean versus Non-Euclidean Gamma-Ray Bursts

TL;DR: In this paper, the authors classify gamma-ray bursts according to their observed durations and physical properties of their spectra, and find that long/hard bursts (of duration T90>2.5 s, and typical photon energy Ep 0.8 MeV, corresponding to BATSE's energy fluence hardness He32>3) show the strongest deviation from the three-dimensional Euclidean brightness distribution.
Journal ArticleDOI

THEORIES OF γ‐RAY BURSTSfn1

TL;DR: Theoretical models of cosmic gamma bursts fall into four categories: extra galactic models, flares, accretion onto collapsed stars, and exotic mechanisms as mentioned in this paper, and factors such as source properties, source dimensions, and radiation mechanisms are considered, in discussing these models.
Journal Article

Gamma-ray bursts from accreting black holes in neutron star mergers

TL;DR: In this article, the formation and the properties of the accretion torus around the stellar mass black hole which originates from the merging of two neutron stars were investigated by means of three-dimensional hydrodynamic simulations with a Eulerian PPM code.
Journal ArticleDOI

Euclidean vs. non-Euclidean Gamma-Ray Bursts

Marco Tavani
- 13 Feb 1998 - 
TL;DR: In this paper, the authors classify gamma-ray bursts (GRBs) according to their observed durations and physical properties of their spectra, and find that long/hard bursts (of duration T_90 > 2.5 s, and typical photon energy E_p > 0.8 MeV corresponding to BATSE's energy fluence hardness H^e_{32} > 3) show the strongest deviation from the three-dimensional Euclidean brightness distribution.
Journal ArticleDOI

Simulations of Gamma-Ray Bursts from External Shocks: Time Variability and Spectral Correlations

TL;DR: In this paper, burst spectra and time structures arising from synchrotron and inverse Compton scattering by nonthermal electrons accelerated in shocks that form during the interaction between a thin ultrarelativistic fireball and a stationary external medium were computed.
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