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The redshift distribution of gamma-ray bursts collected in the BATSE Catalog is compared with the star formation rate. We aim to clarify the accordance between them. We also study the case of comoving number density of bursts monotonously…

Astrophysics · Physics 2009-11-11 A. Meszaros , Z. Bagoly , L. G. Balazs , I. Horvath

In the hadronic fireball phenomenology of Gamma Ray Bursts (GRBs), it is expected that the observed photons are accompanied by UHE neutrinos, which have not been observed yet. It is one of the challenges of experimental UHE neutrino…

Astrophysics · Physics 2009-11-13 Julia K. Becker , Michael Stamatikos , Francis Halzen , Wolfgang Rhode

We show that the time variability of a gamma-ray burst (GRB) appears to be correlated with the absolute luminosity of the burst: smooth bursts are intrinsically less luminous. This Cepheid-like relationship can be used to determine the…

Astrophysics · Physics 2007-05-23 E. E. Fenimore , E. Ramirez-Ruiz

We have tested several models of GRB luminosity and redshift distribution functions for compatibility with the BATSE 4B number versus peak flux relation. Our results disagree with recent claims that current GRB observations can be used to…

Astrophysics · Physics 2009-10-30 Mark R. Krumholz , S. E. Thorsett , Fiona A. Harrison

Identification of gravitationally lensed Gamma Ray Bursts (GRBs) in the BATSE 4B catalog can be used to constrain the average redshift $ < z >$ of the GRBs. In this paper we investigate the effect of evolving lenses on the $< z >$ of GRBs…

Astrophysics · Physics 2009-10-31 Deepak Jain , N. Panchapakesan , S. Mahajan , V. B. Bhatia

Gamma-ray burst (GRB) data suggest that the jets from GRBs in the high redshift universe are more narrowly collimated than those at lower redshifts. This implies that we detect relatively fewer long GRB progenitor systems (i.e. massive…

High Energy Astrophysical Phenomena · Physics 2020-10-07 Nicole M. Lloyd-Ronning , Jarrett L. Johnson , Aycin Aykutalp

We study the peak energy ($E_{\rm{p}}$) distribution of the $\nu F_{\nu}$ spectra of gamma-ray bursts (GRBs) and X-ray flashes (XRFs) with a sample of 57 bursts observed by {\em High Energy Transient Explorer 2} ({\em HETE-2}) French Gamma…

Astrophysics · Physics 2009-11-10 E. W. Liang , Z. G. Dai

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…

General Relativity and Quantum Cosmology · Physics 2015-09-23 Andrzej Krasiński

We extend a previous work on the intrinsic spectral properties and energetics of GRBs with known redshift based on 12 BeppoSAX events by including in the sample a total of 10 more events detected either by BATSE, BeppoSAX or HETE-2. An…

Astrophysics · Physics 2014-10-13 L. Amati

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…

Astrophysics · Physics 2007-05-23 Tomonori TOTANI

The measured redshifts of gamma-ray bursts (GRBs), which were first detected by the Swift satellite, seem to be bigger on average than the redshifts of GRBs detected by other satellites. We analyzed the redshift distribution of GRBs…

High Energy Astrophysical Phenomena · Physics 2009-01-21 Z. Bagoly , L. G. Balazs , I. Horvath , J. Kelemen , A. Meszaros , P. Veres , G. Tusnady

We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first three years of its mission, focusing on the properties of X-Ray Flashes (XRFs) and X-ray-rich GRBs (XRRs). We find that the…

The measured redshifts of gamma-ray bursts (GRBs), which were first detected by the Swift satellite, seem to be bigger on average than the redshifts of GRBs detected by other satellites. We analyzed the redshift distribution of GRBs…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Z. Bagoly , P. Veres

The gamma ray burst apparent average isotropic power versus their red-shift of all known GRB (Sept.2009) is reported. It calls for an unrealistic Gamma Ray Burst Evolution around us or it just probe the need of a very thin gamma…

High Energy Astrophysical Phenomena · Physics 2014-11-20 D. Fargion , D. D'Armiento

We compare the luminosity function and rate inferred from the BATSE long bursts peak flux distribution with those inferred from the Swift peak flux distribution. We find that both the BATSE and the Swift peak fluxes can be fitted by the…

Astrophysics · Physics 2008-11-26 Dafne Guetta , Tsvi Piran

The unrivalled, extreme luminosities of gamma-ray bursts (GRBs) make them the favored beacons for sampling the high redshift Universe. To employ GRBs to study the cosmic terrain -- e.g., star and galaxy formation history -- GRB luminosities…

Astrophysics · Physics 2007-05-23 J. P. Norris

We study the spectrum of the prompt emission and the X-ray and optical afterglow fluxes of 54 X-Ray Rich Gamma Ray Burst (XRRs) and X-Ray Flashes (XRFs), observed by BeppoSax and HETE-2. A comparison is then performed with classical Gamma…

Astrophysics · Physics 2015-06-24 V. D' Alessio , L. Piro , E. M. Rossi

Due to their highly luminous nature, gamma-ray bursts (GRBs) are useful tools in studying the early Universe (up to z = 10). We consider whether the available subset of Swift high redshift GRBs are unusual when compared to analogous…

High Energy Astrophysical Phenomena · Physics 2013-08-27 O. M. Littlejohns , N. R. Tanvir , R. Willingale , P. T. O'Brien , P. A. Evans , A. J. Levan

We employ realistic constraints on astrophysical and instrumental selection effects to model the Gamma-Ray Burst (GRB) redshift distribution using {\it Swift} triggered redshift samples acquired from optical afterglows (OA) and the TOUGH…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 David Coward , Eric Howell , Marica Branchesi , Giulia Strata , Dafne Guetta , Bruce Gendre , Damien Macpherson

New two- and three-dimensional calculations are presented of relativistic jet propagation and break out in massive Wolf-Rayet stars. Such jets are thought responsible for gamma-ray bursts. As it erupts, the jet is surrounded by a cocoon of…

Astrophysics · Physics 2009-11-10 Weiqun Zhang , S. E. Woosley , A. Heger