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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

Relativistic fireballs: energy conversion and time-scales

TL;DR: In this paper, the expansion energy of a relativistic fireball can be reconverted into radiation when it interacts with an external medium, and the corresponding time-scale in the frame of the observer is of the order of seconds.
Journal ArticleDOI

Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray Burst Sources

TL;DR: In this article, the relativistic two-stream instability can naturally generate strong magnetic fields with 10-5-10-1 of the equipartition energy density, in the collisionless shocks of gamma-ray burst (GRB) sources.
Journal ArticleDOI

Are gamma-ray bursts optically thick?

TL;DR: On montre que les sources Rγ peuvent etre optiquement epaisses a la creation de paires si la densite d'energie dans la region emettrice est suffisamment elevee as discussed by the authors.
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