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Related papers: A Gamma-Ray Burst Bibliography, 1973-2001

200 papers

This article reviews the present status of high energy gamma-ray astronomy at energies above 30 MeV. Observations in the past decade using both space- and ground-based experiments have been primarily responsible for giving a tremendous…

Astrophysics · Physics 2010-12-03 R. Mukherjee

Cosmic gamma-ray bursts are one of the great frontiers of astrophysics today. They are a playground of relativists and observers alike. They may teach us about the death of stars and the birth of black holes, the physics in extreme…

We describe observational evidence and theoretical calculations which support the high velocity neutron star model of gamma-ray bursts. We estimate the energetic requirements in this model, and discuss possible energy sources. we also…

Astrophysics · Physics 2009-10-28 Donald Q. Lamb , Tomasz Bulik , Paolo S. Coppi

If gamma-ray bursts have a cosmological origin, the sources are expected to trace the large-scale structure of luminous matter in the universe. I use a new likelihood method that compares the counts-in-cells distribution of gamma-ray bursts…

Astrophysics · Physics 2007-05-23 Jean M. Quashnock

Gamma-ray bursts are the most luminous explosions in the Universe, and their origin as well as mechanism are the focus of intense research and debate. More than three decades since their serendipitous discovery, followed by several…

High Energy Astrophysical Phenomena · Physics 2011-12-06 P. N. Bhat , S. Guiriec

Correlation analysis of Swift gamma-ray burst coordinates and nearby star locations (catalog Gliese) reveals 4 coincidences with good angular accuracy. The random probability is 4\times 10^{-5}, so evidencing that coincident stars are…

High Energy Astrophysical Phenomena · Physics 2011-04-19 B. I. Luchkov

Cosmic explosions called $\gamma$-ray bursts are the most energetic bursting events in the universe. Observations of extremely high-energy emission from two $\gamma$-ray bursts provide a new way to study these gigantic explosions.

High Energy Astrophysical Phenomena · Physics 2020-01-08 Bing Zhang

Gamma-ray bursts are violent events occurring randomly in the sky. In this review, I will present the fireball model, proposed to explain the phenomenon of gamma-ray bursts. This model has important consequences for the production and…

Astrophysics · Physics 2008-07-25 B. Gendre

The gamma ray burst phenomenon is reviewed from a theoretical point of view, with emphasis on the fireball shock scenario of the prompt emission and the longer wavelenght afterglow. Recent progress and issues are discussed, including…

Astrophysics · Physics 2009-11-07 P. Meszaros

I discuss some aspects of the evolution of the standard GRB model, emphasizing various theoretical developments in the last decade, and review the impact of some of the most recent observational discoveries and the new challenges they pose…

High Energy Astrophysical Phenomena · Physics 2019-04-25 P. Mészáros

Gamma-ray bursts (GRBs) are tremendous explosions visible across most of the Universe, certainly out to redshifts of z=4.5 and likely out to z~10. Recently, GRBs have been found to have a roughly constant explosive energy as well as to have…

Astrophysics · Physics 2009-11-07 Bradley E. Schaefer

The origin of cosmic rays is still one of the unresolved questions in modern physics. Violent and high energetic explosions of {\gamma}-ray emission known as Gamma Ray Bursts (GRBs) are perhaps one of the main candidates of sources of…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 Juan A. Aguilar

Gamma Ray Bursts (GRBs) are unpredictable and brief flashes of gamma rays that occur about once a day in random locations in the sky. Since gamma rays do not penetrate the Earth's atmosphere, they are detected by satellites, which…

High Energy Astrophysical Phenomena · Physics 2015-06-05 A. Gomboc

Gamma-ray bursts are the most luminous explosions in the Universe. They appear connected to supernova remnants from massive stars or the merger of their remnants, and their brightness makes them temporarily detectable out to the larges…

High Energy Astrophysical Phenomena · Physics 2014-01-22 P. Meszaros , M. J. Rees

The last half-century has seen dramatic developments in gamma-ray telescopes, from their initial conception and development through to their blossoming into full maturity as a potent research tool in astronomy. Gamma-ray telescopes are…

Instrumentation and Methods for Astrophysics · Physics 2015-05-13 N. Gehrels , J. K. Cannizzo

We collect information as complete as possible about the upcoming telescopes and facilities relevant to gamma-ray bursts, both in the electromagnetic bands as well as for non-electromagnetic messengers. We describe the expected synergy…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-22 Jochen Greiner , Arne Rau

Gamma-ray bursts are the most luminous and probably the most relativistic events in the universe. The last few years have seen a tremendous increase in our knowledge of these events, but the source of the bursts still remains elusive. I…

Astrophysics · Physics 2007-05-23 Stephan Rosswog

Gamma-ray bursts are the most concentrated explosions in the Universe. They have been detected electromagnetically at energies up to tens of GeV, and it is suspected that they could be active at least up to TeV energies. It is also…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Péter Mészáros , Katsuaki Asano , Péter Veres

Gamma-ray bursts (GRBs) are bright flashes of gamma-rays coming from the cosmos. They occur roughly once per day, last typically 10s of seconds and are the most luminous events in the universe. More than three decades after their discovery,…

High Energy Astrophysical Phenomena · Physics 2012-09-03 Neil Gehrels , Peter Meszaros

Gamma-ray burst sources are distributed with a high level of isotropy, which is compatible with either a cosmological origin or an extended Galactic halo origin. The brightness distribution is another indicator used to characterize the…

High Energy Astrophysical Phenomena · Physics 2015-05-26 I. Horvath