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Related papers: Gamma-Ray Burst - Supernova Relation

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Relativistic supernovae have been discovered until recently only through their association with long duration Gamma Ray Bursts (GRB). As the ejecta mass is negligible in comparison to the swept up mass, the blastwaves of such explosions are…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Sayan Chakraborti , Alak Ray

This paper presents the theoretical basis of the fireball/blast wave model, and some implications of recent results on GRB source models and cosmic-ray production from GRBs. BATSE observations of the prompt gamma-ray luminous phase, and…

Astrophysics · Physics 2007-05-23 C. D. Dermer

The probability of observing "supernova - gamma-ray burst" (GRB) pair events and recurrent GRBs from one galaxy in a time interval of several years has been estimated. Supernova explosions in binary systems accompanied by the formation of a…

High Energy Astrophysical Phenomena · Physics 2011-02-22 V. I. Dokuchaev , Yu. N. Eroshenko

Context: Observations suggest that the major fraction of long duration gamma-ray bursts (GRBs) are connected with broad-lines supernovae Ib/c, (SNe-Ibc). The presence of GRB-SNe is revealed by rebrightenings emerging from the optical GRB…

High Energy Astrophysical Phenomena · Physics 2014-10-01 M. Kovacevic , L. Izzo , Y. Wang , M. Muccino , M. Della Valle , L. Amati , C. Barbarino , M. Enderli , G. B. Pisani , L. Li

The Gamma-Ray Bursts - GRBs are one of the most energetic astronomical events in the universe that have not yet an adequate explanation of what kind of mechanism is carried out. This question motivates the astronomical community to do…

High Energy Astrophysical Phenomena · Physics 2013-07-05 Camilo Delgado-Correal

It has been observationally established that supernovae (SNe) of Type Ic produce long duration gamma ray bursts (GRBs) and that neutron star mergers generate short hard GRBs. SN-Less GRBs presumably originate in a phase transition of a…

High Energy Astrophysical Phenomena · Physics 2022-07-06 Shlomo Dado , Arnon Dar , A. De Rújula

Afterglow, or long-lived emission, has now been detected from about a dozen well-positioned gamma-ray bursts. Distance determinations made by measuring optical emission lines from the host galaxy, or absorption lines in the afterglow…

Much of progress in gamma-ray bursts has come from the studies of distant events (redshift z~1). The brightest GRBs are the most collimated events and seen across the Universe due to their brilliance. It has long been suspected that nearest…

Astrophysics · Physics 2009-11-10 S. Sazonov , A. Lutovinov , R. Sunyaev

Gamma-ray bursts (GRBs) are the most violent explosions in the Universe and can be used to explore the properties of high-redshift universe. It is believed that the long GRBs are associated with the deaths of massive stars. So it is…

High Energy Astrophysical Phenomena · Physics 2015-05-27 H. Yu , F. Y. Wang , Z. G. Dai , K. S. Cheng

We use the BD2 sample of gamma-ray bursts (GRBs) based on 5.9 years of BATSE DISCLA data with a variety of models of the luminosity function to derive characteristic GRB luminosities, space densities and redshift distributions. Previously…

Astrophysics · Physics 2009-10-31 Maarten Schmidt

Since the launch of the highly successful and ongoing Swift mission, the field of gamma-ray bursts (GRBs) has undergone a revolution. The arcsecond GRB localizations available within just a few minutes of the GRB alert has signified the…

Astrophysics of Galaxies · Physics 2017-09-26 Patricia Schady

It has been suggested that cosmological gamma-ray bursts (GRBs) can produce the observed flux and spectrum of cosmic rays at the highest energies. However, recent observations indicate that the redshift distribution of GRBs most likely…

Astrophysics · Physics 2011-05-23 F. W. Stecker

Long gamma-ray bursts (LGRBs) are typically thought to result from the collapse of massive stars. Nonetheless, recent observations of gamma-ray bursts (GRBs) 211211A and 230307A, coupled with the low-redshift excess of LGRB event rates…

High Energy Astrophysical Phenomena · Physics 2025-05-12 Yan-Kun Qu , Zhong-Xiao Man , Zhi-Bin Zhang

I present an analysis of the gamma-ray and afterglow energies of the complete sample of 17 short duration GRBs with prompt X-ray follow-up. I find that 80% of the bursts exhibit a linear correlation between their gamma-ray fluence and the…

Astrophysics · Physics 2009-11-13 E. Berger

Gamma-ray bursts (GRBs) are the most luminous explosions in the universe, yet the nature and physical properties of their energy sources are far from understood. Very important clues, however, can be inferred by studying the afterglows of…

Since their identification with cosmological distances, Gamma-ray bursts (GRBs) have been recognised as the most energetic phenomena in the Universe, with an isotropic burst energy as high as 10^54 ergs. However, the progenitors responsible…

Gamma-ray Bursts (GRBs) generate powerful relativistic jets that inject a large amount of energy into their surrounding environment, producing blast waves that accelerate particles to high energies. The GRB afterglow radiation provides a…

High Energy Astrophysical Phenomena · Physics 2026-02-24 P. Tiwari , B. Banerjee , D. Miceli , G. Oganesyan , A. Ierardi , S. Macera , M. Branchesi , L. Nava , S. Mohnani , S. Agarwal , A. Shukla

Gamma-ray bursts GRBs are among the most mysterious astronomical phenomenon ever discovered. Unlike most astronomical discoveries which were explained within weeks or months after their initial discovery, GRBs remain a puzzle for more than…

Astrophysics · Physics 2007-05-23 Tsvi Piran

Gamma-ray bursts (GRBs) are extremely powerful explosions that have been traditionally classified into two categories: long bursts (LGRBs) with an observed duration T90 > 2 s, and short bursts (SGRBs) with an observed duration T90 < 2 s,…

High Energy Astrophysical Phenomena · Physics 2024-03-25 Ali M. Hasan , Walid J. Azzam

Gamma-ray bursts (GRBs) are violent explosions, coming from cosmological distances. They are detected in gamma-rays (also X-rays, UV, optical, radio) almost every day, and have typical durations of a few seconds to a few minutes. Some GRBs…

High Energy Astrophysical Phenomena · Physics 2015-06-10 Antonios Nathanail , Ioannis Contopoulos