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The distribution of the apparent total energy emitted by a gamma-ray burst reflects not only the distribution of the energy actually released by the burst engine, but also the distribution of beaming angles. Using the observed energy…

天体物理学 · 物理学 2009-11-06 David L. Band

The energy release in gamma-ray bursts is one of the most interesting clues on the nature of their "inner engines". We show here that the total energy release in GRBs varies by less than one order of magnitude from one burst to another…

天体物理学 · 物理学 2007-05-23 Tsvi Piran , Pawan Kumar , Alin Panaitescu , Luigi Piro

We predict the redshift distribution of Gamma-Ray Bursts (GRBs) assuming that they trace the cosmic star formation history. We find that a fraction >~50% of all GRBs on the sky originate at a redshift z >~5, even though the fraction of the…

天体物理学 · 物理学 2011-07-19 Volker Bromm , Abraham Loeb

The energy of a Gamma-Ray Burst is one of the most interesting factors that can help determining the origin of these mysterious explosions. After the discovery that GRBs are cosmological it was thought, for a while that they are standard…

天体物理学 · 物理学 2007-05-23 Tsvi Piran

We show that the distribution of observed energies of GRB with known redshifts can be explained by the hypothesis of the standard energy release E_0=5 10^51 ergs. Two situations are possible, either the beaming angle differs from burst to…

天体物理学 · 物理学 2009-10-31 K. A. Postnov , M. E. Prokhorov , V. M. Lipunov

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

天体物理学 · 物理学 2009-10-31 S. T. Scully , F. W. Stecker

The determination of the luminosity function (LF) in gamma ray bursts (GRBs) depends on the adopted cosmology, each one characterized by its corresponding luminosity distance. Here we analyse three cosmologies: the standard cosmology, the…

宇宙学与河外天体物理 · 物理学 2016-11-08 L. Zaninetti

Gamma ray bursts (GRBs) are known to have short-time variability and power-law behavior with the index -1.67 in the power spectrum density. Reanalyzing the expanded data, we have found a) the power-law comes from the global profile of the…

天体物理学 · 物理学 2009-11-06 Motoko Suzuki , Masahiro Morikawa , Izumi Joichi

Gamma Ray Bursts (GRBs) are among the most powerful sources in the Universe: they emit up to 10^54 erg in the hard X-ray band in few tens of seconds. The cosmological origin of GRBs has been confirmed by several spectroscopic measurements…

天体物理学 · 物理学 2011-07-19 G. Ghirlanda , G. Ghisellini , C. Firmani

Gamma Ray Bursts (GRBs) are notorious for their diversity. Yet, they have a series of common features. The typical energy of their $\gamma$ rays is a fraction of an MeV. The energy distributions are well described by a ``Band spectrum'',…

天体物理学 · 物理学 2009-11-10 Arnon Dar , A. De Rujula

In the external shock model, gamma-ray burst (GRB) emissions are produced by the energization and deceleration of a thin relativistic blast wave due to its interactions with the circumburst medium (CBM). We study the physical properties of…

天体物理学 · 物理学 2009-10-31 Charles D. Dermer , Markus Boettcher , J. Chiang

A temporal analysis has been performed on a sample of 100 bright gamma-ray bursts (GRBs) with T90<2s from the BATSE current catalog. The GRBs were denoised using a median filter and subjected to an automated pulse selection algorithm as an…

天体物理学 · 物理学 2009-11-07 S. McBreen , F. Quilligan , B. McBreen , L. Hanlon , D. Watson

Discovered more than 50 years ago, gamma-ray burst (GRB) prompt emission remains the most puzzling aspect of GRB physics. Its complex and irregular nature should reveal how newborn GRB engines release their energy. In this respect, the…

高能天体物理现象 · 物理学 2024-01-26 R. Maccary , C. Guidorzi , L. Amati , L. Bazzanini , M. Bulla , A. E. Camisasca , L. Ferro , F. Frontera , A. Tsvetkova

A hypothesis is proposed that the gamma-ray bursts (GRBs) may arise by blueshifting the emission radiation of hydrogen and helium generated during the last scattering epoch. The blueshift mechanism is provided by such a Lema\^itre -- Tolman…

广义相对论与量子宇宙学 · 物理学 2015-09-23 Andrzej Krasiński

A gamma-ray burst (GRB) releases an amount of energy similar to that of a supernova explosion, which combined with its rapid variability suggests an origin related to neutron stars or black holes. Since these compact stellar remnants form…

天体物理学 · 物理学 2020-11-25 Ralph A. M. J. Wijers , Joshua S. Bloom , Jasjeet S. Bagla , Priyamvada Natarajan

The observational diversity of ``gamma-ray bursts'' (GRBs) has been increasing, and the natural inclination is a proliferation of models. We explore the possibility that at least part of this diversity is a consequence of a single basic…

天体物理学 · 物理学 2008-11-26 S. E. Woosley , Weiqun Zhang

Observations of individual bursts chosen by the vagaries of telescope availability demonstrated that bursts are not standard candles and that their apparent energy can be as great as 10^54 erg. However, determining the distribution of their…

天体物理学 · 物理学 2009-11-06 David L. Band

Selection effects, connected with stochastic errors in source flux and threshold value determination are analyzed. Normal and normal logarithmic distributions of stochastic deviations are considered. These two kind of distributions produce…

天体物理学 · 物理学 2007-05-23 G. S. Bisnovatyi-Kogan

The present common view about GRB origin is related to cosmology. There are two evidences in favour of this interpretation. The first is connected with statistics, the second is based on measurements of the redshifts in the GRB optical…

天体物理学 · 物理学 2009-11-06 G. S. Bisnovatyi-Kogan

Gamma-ray bursts (GRBs) are the most brilliant objects in the Universe but efforts to estimate the total energy released in the explosion -- a crucial physical quantity -- have been stymied by their unknown geometry: spheres or cones. We…

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