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相关论文: On the nature of gamma-ray burst time dilations

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The recent discovery that faint gamma-ray bursts are stretched in time relative to bright ones has been interpreted as support for cosmological distances: faint bursts have their durations redshifted relative to bright ones. It was pointed…

天体物理学 · 物理学 2009-10-22 Ralph A. M. J. Wijers , Bohdan Paczyński

The isotropic distribution of gamma-ray bursts as observed with the Burst and Transient Experiment (BATSE) strongly suggests that the bursts are at cosmological distances. At such distances, the expansion of the universe should redshift the…

天体物理学 · 物理学 2009-10-28 Ed E. Fenimore , Joshua S. Bloom

If gamma-ray bursters are at cosmological distances - as suggested by their isotropic distribution on the sky and by their number-intensity relation - then the burst profiles will be stretched in time, by an amount proportional to the…

Gamma-Ray Bursts have been observed out to very high redshifts and provide time measures that are directly related to intrinsic time scales of the burst. Einstein's theory of relativity is quite definite that if the universe is expanding…

综合物理 · 物理学 2010-09-12 David F. Crawford

Norris et al. (1994) report that the temporal structure of faint gamma ray bursts is longer than that of bright bursts, as expected for time dilation in the cosmological models of burst origin. I show that the observed trends can easily be…

天体物理学 · 物理学 2009-10-22 David Band

Several claims have been put forward that an essential fraction of long-duration BATSE gamma-ray bursts should lie at redshifts larger than 5. This point-of-view follows from the natural assumption that fainter objects should, on average,…

宇宙学与河外天体物理 · 物理学 2015-05-27 Attila Meszaros , Jakub Ripa , Felix Ryde

If $\gamma$-ray bursts are at cosmological distances, then not only their constituent pulses but also the intervals between pulses should be time-dilated. Unlike time-dilation measures of pulse emission, intervals would appear to require…

天体物理学 · 物理学 2009-10-28 J. P. Norris , J. T. Bonnell , R. J. Nemiroff , J. D. Scargle

Several claims have been put forward that an essential fraction of long-duration BATSE gamma-ray bursts should lie at redshifts larger than 5. This point-of-view follows from the natural assumption that fainter objects should, on average,…

高能天体物理现象 · 物理学 2012-09-13 Jakub Ripa , Attila Meszaros , Felix Ryde

The positions of over 1000 gamma-ray bursts detected with the BATSE experiment on board of the Compton Gamma Ray Observatory are uniformly and randomly distributed in the sky, with no significant concentration to the galactic plane or to…

天体物理学 · 物理学 2016-08-30 Bohdan Paczynski

We find that dim gamma-ray bursts (GRBs) are softer than bright GRBs, as indicated on average by data from the Burst and Transient Source Experiment (BATSE) on board the Compton Gamma Ray Observatory. We show that this correlation is…

Several hundred gamma-ray burst (GRB) redshifts have been determined to date. One of the other important properties-besides the distance-of the GRBs is the duration of the burst. In this paper, we analyse these two important quantities of…

高能天体物理现象 · 物理学 2022-06-30 I. Horvath , I. I. Racz , Z. Bagoly , L. G. Balazs , S. Pinter

We argue that the distributions of both the intrinsic fluence and the intrinsic duration of the gamma-ray emission in gamma-ray bursts from the BATSE sample are well represented by log-normal distributions, in which the intrinsic dispersion…

天体物理学 · 物理学 2011-05-23 L. G. Balazs , Z. Bagoly , I. Horvath , A. Meszaros , P. Meszaros

We observe strong correlations between the temporal properties of gamma ray bursts (GRBs) and their apparent peak brightness. The strongest effect (with a significance level of 10^{-6}) is the difference between the brightness distributions…

天体物理学 · 物理学 2011-07-13 Boris Stern , Juri Poutanen , Roland Svensson

Brightness dependent correlations have been conclusively detected in the average time profiles of gamma-ray bursts (GRBs). Determining the time constants of the stretched exponential slopes of the average peak-aligned time profile of GRBs…

天体物理学 · 物理学 2009-10-30 Boris Stern , Juri Poutanen , Roland Svensson

Cosmological time dilation is a fundamental phenomenon in an expanding universe, which stresses that both the duration and wavelength of the emitted light from a distant object at the redshift $z$ will be dilated by a factor of $1+z$ at the…

高能天体物理现象 · 物理学 2013-11-08 Fu-Wen Zhang , Yi-Zhong Fan , Lang Shao , Da-Ming Wei

The time profiles of many gamma-ray bursts consist of distinct pulses, which offers the possibility of characterizing the temporal structure of these bursts using a relatively small set of pulse shape parameters. We have used a pulse…

天体物理学 · 物理学 2014-10-13 Andrew Lee , Elliott D. Bloom , Vahe Petrosian

In order to explain the origin of skewness in the gamma-ray burst (GRB) duration distribution, a statistical model, based on the cosmological time dilation and taking into account the GRB formation rate and instrumental effects, is…

高能天体物理现象 · 物理学 2020-07-15 Mariusz Tarnopolski

From recent observations of gamma-ray bursts (GRBs), it appears that spectral time lags between higher-energy gamma rays photons and lower-energy photons vary with energy difference and time (distance) traveled. These lags appear to be…

天体物理学 · 物理学 2010-04-05 Theodore G. Pavlopoulos

We perform several nonparametric correlation tests on the BATSE 3B data to search for evidence of cosmological time dilation. These tests account for the effects of data truncation due to threshold effects in both limiting brightness and…

天体物理学 · 物理学 2009-10-28 Theodore T. Lee , Vahe Petrosian

We argue that the distributions of both the intrinsic fluence and the intrinsic duration of the gamma-ray emission in gamma-ray bursts from the BATSE sample are well represented by log-normal distributions, in which the intrinsic dispersion…

天体物理学 · 物理学 2007-05-23 L. G. Balazs , P. Meszaros , Z. Bagoly , I. Horvath , A. Meszaros
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