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相关论文: Are Gamma-Ray Bursts Standard Candles?

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The measure of the distances and luminosities of gamma-ray bursts (GRBs) led to the discovery that many GRB properties are strongly correlated with their intrinsic luminosity, leading to the construction of reliable luminosity indicators.…

天体物理学 · 物理学 2010-11-11 J-L. Atteia

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

It is often stated that gamma-ray bursts (GRBs) have typical energies of several hundred keV. Is this a real feature of GRBs or is it due to an observational bias? We consider the possibility that bursts of a given bolometric luminosity…

天体物理学 · 物理学 2009-10-28 Tsvi Piran , Ramesh Narayan

Two different luminosity indicators have recently been proposed for Gamma Ray Bursts that use gamma-ray observations alone. They relate the burst luminosity (L) with the time lag between peaks in hard and soft energies, and the spikiness or…

天体物理学 · 物理学 2009-11-06 Bradley E. Schaefer , Ming Deng , David L. Band

Gamma-ray bursts (GRB) are short and intense bursts of $\sim$100 keV$-$1MeV photons, usually followed by long-lasting decaying afterglow emission in a wide range of electromagnetic wavelengths from radio to X-ray and, sometimes, even to GeV…

高能天体物理现象 · 物理学 2023-04-05 Yun-Wei Yu , He Gao , Fa-Yin Wang , Bin-Bin Zhang

Long duration gamma-ray bursts (GRB) are at cosmological distance, they appear to be located near star forming regions, and are likely associated with some type of supernovae. They are also likely to be strongly beamed, which lowers their…

天体物理学 · 物理学 2007-05-23 Bohdan Paczynski

We show that if the intrinsic break energy of Gamma-Ray Bursts (GRBs) is determined by the product of more than three random variables the observed break energy distribution becomes almost lognormal including the redshift effect because of…

天体物理学 · 物理学 2009-11-07 Kunihito Ioka , Takashi Nakamura

It has been argued that the long gamma-ray burst (GRB) of GRB 060614 without an associated supernova (SN) has challenged the current classification and fuel model for long GRBs, and thus a tidal disruption model has been proposed to account…

高能天体物理现象 · 物理学 2010-06-17 H. Gao , Y. Lu , S. N. Zhang

Two different multivariate clustering techniques, the K-means partitioning method and the Dirichlet process of mixture modeling, have been applied to the BATSE Gamma-ray burst (GRB) catalog, to obtain the optimum number of coherent groups.…

天体物理学 · 物理学 2010-06-22 Tanuka Chattopadhyay , Ranjeev Misra , Asis Kumar Chattopadhyay , Malay Naskar

Ultra-long Gamma-Ray Bursts are a class of high energy transients lasting several hours. Their exact nature is still elusive, and several models have been proposed to explain them. Because of the limited coverage of wide field gamma-ray…

高能天体物理现象 · 物理学 2019-06-03 B. Gendre , Q. T. Joyce , N. B. Orange , G. Stratta , J. L. Atteia , M. Boer

The variable activity of a gamma-ray burst (GRB) source is thought to be correlated with its absolute peak luminosity - a relation that, if confirmed, can be used to derive an independent estimate of the redshift of a GRB. We find that…

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

The separation of the gamma-ray bursts (GRBs) into short/hard and long/soft subclasses, respectively, is well supported both theoretically and observationally. The long ones are coupled to supernovae type Ib/Ic - the short ones are…

高能天体物理现象 · 物理学 2020-01-06 Attila Mészáros , Jakub Řípa

A sample of 18 long-lag (tau_{lag} > 1 s) Gamma-Ray Bursts (GRBs) has been drawn from our catalog of all Swift long GRBs. Four different tests are done on this sample to test the prediction that a large fraction of long-lag GRBs are from…

宇宙学与河外天体物理 · 物理学 2014-11-18 Limin Xiao , Bradley E. Schaefer

With the understanding that the enigmatic Gamma-Ray Burts (GRBs) are beamed explosions, and with the recently discovered ``Ghirlanda-relation'', the dream of using GRBs as cosmological yardsticks may have come a few steps closer to reality.…

天体物理学 · 物理学 2009-07-29 E. Mortsell , J. Sollerman

Gamma rays from extragalactic sources are attenuated by pair-production interactions with diffuse photons of the extragalactic background light (EBL). Gamma-ray bursts (GRBs) are a source of high-redshift photons above 10 GeV, and could be…

宇宙学与河外天体物理 · 物理学 2015-05-14 Rudy C. Gilmore , Francisco Prada , Joel R. Primack

We discuss some open problems concerning the origin and the emission mechanism of gamma-ray bursts (GRBs) in light of recent developments. If GRBs originate at extragalactic distances, we are facing four crises: (1) an energy crisis, models…

天体物理学 · 物理学 2007-05-23 Marco Tavani

Gamma-ray bursts (GRBs) are traditionally classified into long (lGRBs) and short (sGRBs) durations based on their $T_{90}$, with lGRBs widely used as tracers of the cosmic star formation rate (SFR) due to their observed association with…

高能天体物理现象 · 物理学 2025-09-15 Qin-Mei Li , Qi-Bin Sun , Sheng-Bang Qian , Fu-Xing Li

We investigate whether Gamma-Ray Bursts (GRBs) from the Current BATSE Catalog have been affected by weak lensing by the nearby large scale structure. The redshift distribution of GRBs is believed to be broad, extending to z~5, so most…

天体物理学 · 物理学 2011-07-19 Liliya L. R. Williams , Natalie Frey

Correlations among pulse properties in the prompt emission of long GRBs can potentially be used as cosmological distance indicators to estimate redshifts of GRBs to which these pulses belong. We demonstrate application of this technique to…

高能天体物理现象 · 物理学 2009-06-25 Jon Hakkila , P. Chris Fragile , Timothy W. Giblin

Gamma-ray bursts (GRBs) are a potential tool to probe high-redshift universe. However, the circularity problem enforces people to find model-independent methods to study the luminosity correlations of GRBs. Here, we present a new method…

高能天体物理现象 · 物理学 2019-03-06 Yu-Yang Wang , F. Y. Wang
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