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Most of proposed models of cosmological gamma-ray bursts (GRBs) are associated to gravitational collapses of massive stars, and hence evolution of the GRB rate, which is crucially important in GRB intensity distribution analysis, is…

天体物理学 · 物理学 2007-05-23 Tomonori TOTANI

A critical comparison of estimates for the rates of hypernovae (HNe) and gamma-ray bursts (GRBs) is presented. Within the substantial uncertainties, the estimates are shown to be quite comparable and give a Galactic rate of $10^{-6}$ --…

天体物理学 · 物理学 2011-06-21 Ph. Podsiadlowski , P. A. Mazzali , K. Nomoto , D. Lazzati , E. Cappellaro

A planet having protective ozone within the collimated beam of a Gamma Ray Burst (GRB) may suffer ozone depletion, potentially causing a mass extinction event to existing life on a planet's surface and oceans. We model the dangers of long…

地球与行星天体物理 · 物理学 2016-11-23 Michael G. Gowanlock

The data on the location of gamma-ray bursts (GRBs) relative to their host galaxies are used to derive the distribution of surface density of GRBs along the galaxy radius. It is shown that the gradient of GRB surface density changes…

天体物理学 · 物理学 2007-05-23 D. Yu. Tsvetkov , S. I. Blinnikov , N. N. Pavlyuk

The association of long gamma-ray bursts with supernovae naturally suggests that the cosmic GRB rate should trace the star formation history. Finding otherwise would provide important clues concerning these rare, curious phenomena. Using a…

天体物理学 · 物理学 2010-11-11 Matthew D. Kistler , Hasan Yuksel , John F. Beacom , Krzysztof Z. Stanek

Brightness distribution of Gamma-Ray Bursts (GRBs) is studied in detail under the assumption that GRB rate is related to cosmic star formation rate. The two populations of the long- and short-duration bursts in the 4B BATSE catalog are…

天体物理学 · 物理学 2009-10-30 Tomonori Totani

Based on a simulation of galaxy formation in the standard cosmological model, we suggest that a consistent picture for Gamma-Ray Bursts and star formation may be found that is in broad agreement with observations: GRBs preferentially form…

天体物理学 · 物理学 2007-10-25 Renyue Cen , Taotao Fang

Motivated by the recent observational and theoretical evidence that long Gamma-Ray Bursts (GRBs) are likely associated with low metallicity, rapidly rotating massive stars, we examine the cosmological star formation rate (SFR) below a…

天体物理学 · 物理学 2009-11-13 A. Lapi , N. Kawakatu , Z. Bosnjak , A. Celotti , A. Bressan , G. L. Granato , L. Danese

Recent evidence appears to link gamma-ray bursts (GRBs) to star-forming regions in galaxies at cosmological distances. If short-lived massive stars are the progenitors of GRBs, the rate of events per unit cosmological volume should be an…

天体物理学 · 物理学 2008-11-26 Cristiano Porciani , Piero Madau

As starburst galaxies show a star formation rate up to several hundred times larger than the one in a typical galaxy, the expected supernova rate is higher than average. This in turn implies a high rate of long gamma ray bursts (GRBs),…

高能天体物理现象 · 物理学 2009-09-14 Jens Dreyer , Julia K. Becker , Wolfgang Rhode

We measure the local rates of ``low-luminosity'' (LL-GRBs, i.e. L<10^{48--49}erg/sec) and ``high-luminosity'' Gamma-ray Bursts (HL-GRBs). The values are in the range n0=100--1800 Gpc^(-3)yr^(-1) and n0=100--550 Gpc^(-3) yr^(-1),…

天体物理学 · 物理学 2009-01-19 Dafne Guetta , Massimo Della Valle

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…

天体物理学 · 物理学 2009-10-31 Maarten Schmidt

Gamma ray bursts (GBRs) are a class of highly energetic explosions emitting radiation in a very short timescale of a few seconds and with a very narrow opening angle. Although, all GRBs observed so far are extragalactic in origin, there is…

高能天体物理现象 · 物理学 2014-03-06 Dimitra Atri , Adrian L. Melott , Andrew Karam

Evolution of the rate density of cosmological gamma-ray bursts (GRBs) is calculated and compared to the BATSE brightness distribution in the context of binary neutron-star mergers as the source of GRBs, taking account of the realistic star…

天体物理学 · 物理学 2010-04-06 Tomonori Totani

Gamma-Ray Bursts (GRBs) are thought to originate at cosmological distances from the most powerful explosions in the Universe. If GRBs are not beamed then the distribution of their number as a function of Gamma-ray flux implies that they…

天体物理学 · 物理学 2009-10-30 Abraham Loeb , Rosalba Perna

We present a systematic search for short-duration gamma-ray bursts (GRBs) in the local Universe based on 14 years of observations with the Neil Gehrels Swift Observatory. We cross-correlate the GRB positions with the GLADE catalogue of…

高能天体物理现象 · 物理学 2020-02-12 S. Dichiara , E. Troja , B. O'Connor , F. E. Marshall , P. Beniamini , J. K. Cannizzo , A. Y. Lien , T. Sakamoto

The cosmic gamma-ray burst (GRB) formation rate, as derived from the variability-luminosity relation for long-duration GRBs, is compared with the cosmic star formation rate. If GRBs are related to the collapse of massive stars, one expects…

天体物理学 · 物理学 2009-10-31 Enrico Ramirez-Ruiz , Edward E. Fenimore , Neil Trentham

Using 220 Gamma-Ray Burst (GRB) redshifts and luminosities derived from the luminosity-variability relationship of Fenimore & Ramirez-Ruiz (2000), we show that there exists a significant correlation between the GRB luminosity and redshift.…

天体物理学 · 物理学 2009-11-07 Nicole M. Lloyd-Ronning , Chris L. Fryer , Enrico Ramirez-Ruiz

Gamma Ray Bursts (GRBs) and galaxies at high redshift represent complementary probes of the star formation history of the Universe. In fact, both the GRB rate and the galaxy luminosity density are connected to the underlying star formation.…

宇宙学与河外天体物理 · 物理学 2015-06-16 M. Trenti , R. Perna , S. Tacchella

A simple physical model for long-duration gamma ray bursts (GRBs) is used to fit the redshift (z) and the jet opening-angle distributions measured with earlier GRB missions and with Swift. The effect of different sensitivities for GRB…

天体物理学 · 物理学 2011-02-11 Truong Le , Charles D. Dermer
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