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相关论文: Uncovering the Intrinsic Variability of Gamma-ray …

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Gamma-ray bursts (GRB) are extremely energetic events and produce highly diverse light curves. Light curves are believed to be resulting from internal shocks reflecting the activities of the GRB central engine. Hence their temporal studies…

高能天体物理现象 · 物理学 2013-07-30 P. N. Bhat

Gamma-ray bursts (GRB) are extremely energetic events and produce highly diverse light curves. Light curves are believed to be resulting from internal shocks reflecting the activities of the GRB central engine. Hence their temporal studies…

高能天体物理现象 · 物理学 2015-06-12 Narayana P. Bhat

The minimum variability timescale (MVT) is a key observable used to probe the central engines of Gamma-Ray Bursts (GRBs) by constraining the emission region size and the outflow Lorentz factor. However, its interpretation is often…

高能天体物理现象 · 物理学 2026-02-13 S. Bala , P. Veres , A. Goldstein , R. Sonawane , R. Samanta , S. Iyyani

We have investigated the time variations in the light curves from a sample of long and short Fermi/GBM Gamma ray bursts (GRBs) using an impartial wavelet analysis. The results indicate that in the source frame, the variability time scales…

高能天体物理现象 · 物理学 2015-06-03 G. A. MacLachlan , A. Shenoy , E. Sonbas , K. S. Dhuga , B. Cobb , T. N. Ukwatta , D. C. Morris , A. Eskandarian , L. C. Maximon , W. C. Parke

Intrinsic variability was searched for in arrival times of six gamma-ray bursts (GRBs) at high energies -- between 30 MeV and 2 GeV -- detected by the Fermi satellite's Large Area Telescope (LAT). The GRBs were selected from the Fermi LAT…

高能天体物理现象 · 物理学 2024-07-31 E. Casey Aldrich , Robert J. Nemiroff

We constrain the minimum variability timescales for 938 GRBs observed by the Fermi/GBM instrument prior to July 11, 2012. The tightest constraints on progenitor radii derived from these timescales are obtained from light curves in the…

高能天体物理现象 · 物理学 2015-10-07 V. Zach Golkhou , Nathaniel R. Butler , Owen M. Littlejohns

We present the results of our study of the variability time scales of a sample of 27 long Swift Gamma-Ray Bursts (GRBs) with known redshifts. The variability time scale can help our understanding of fundamental GRB parameters such as the…

We have developed a computer model to calculate gamma ray burst (GRB) light curves and efficiencies from the interaction of a single, thin blast wave with clouds in the external medium. Large amplitude, spiky variability occurs when the…

天体物理学 · 物理学 2009-10-31 Charles D. Dermer , Kurt E. Mitman

Context. Gamma-ray bursts (GRBs) have traditionally been classified by duration into long (LGRBs) and short (SGRBs), with the former believed to originate from massive star collapses and the latter from compact binary mergers. However,…

高能天体物理现象 · 物理学 2025-10-15 R. Maccary , C. Guidorzi , A. E. Camisasca , M. Maistrello , S. Kobayashi , L. Amati , L. Bazzanini , M. Bulla , L. Ferro , F. Frontera , A. Tsvetkova

In some models of quantum gravity, space-time is thought to have a foamy structure with non-trivial optical properties. We probe the possibility that photons propagating in vacuum may exhibit a non-trivial refractive index, by analyzing the…

天体物理学 · 物理学 2008-11-26 J. Ellis , N. E. Mavromatos , D. V. Nanopoulos , A. S. Sakharov

We present a direct link between the minimum variability time scales extracted through a wavelet decomposition and the rise times of the shortest pulses extracted via fits of 34 Fermi GBM GRB light curves comprised of 379 pulses. Pulses…

高能天体物理现象 · 物理学 2015-06-04 G. A. MacLachlan , A. Shenoy , E. Sonbas , K. S. Dhuga , A. Eskandarian , L. C. Maximon , W. C. Parke

The dissipation process of GRB prompt emission is still unknown. Study of temporal variability may provide a unique way to discriminate the imprint of the inner engine activity from geometry and propagation related effects. We define the…

At the dawn of the gamma-ray burst (GRB) afterglow era, a Cepheid-like correlation was discovered between time variability V and isotropic-equivalent peak luminosity Liso of the prompt emission of about a dozen long GRBs with measured…

We consider whether the variability properties of Gamma-Ray Bursts (GRBs) that produce bright optical and longer wavelength transient afterglows (A-GRBs) are the same as a larger, inclusive sample of bright, long-duration GRBs, selected…

天体物理学 · 物理学 2009-11-10 Joseph A. Munoz , Jonathan C. Tan

The minimum variation timescale (MVT) of soft gamma-ray repeaters can be an important probe to estimate the emission region in pulsar-like models, as well as the Lorentz factor and radius of the possible relativistic jet in gamma-ray burst…

We show that simple kinematic arguments can give limits on the timescale and amplitude of variabilities in gamma-ray burst (GRB) afterglows, especially when the variability timescale is shorter than the observed time since the burst \Delta…

天体物理学 · 物理学 2009-11-10 Kunihito Ioka , Shiho Kobayashi , Bing Zhang

We carry out a search for signatures of cosmological time dilation in the light curves of Gamma Ray Bursts (GRBs), detected by the Neil Gehrels Swift Observatory. For this purpose, we calculate two different durations ($T_{50}$ and…

高能天体物理现象 · 物理学 2022-02-07 Amitesh Singh , Shantanu Desai

A popular paradigm to explain the rapid temporal variability observed in gamma-ray burst (GRB) lightcurves is the internal shock model. We propose an alternative model in which the radiating fluid in the GRB shell is relativistically…

天体物理学 · 物理学 2009-11-13 Ramesh Narayan , Pawan Kumar

We have carried out a detailed study of the morphology of gamma-ray bursts (GRBs) with time duration less than 100 ms that includes: (1) a fast-Fourier spectrum analysis, (2) a comparison with the Stern analysis of longer bursts, (3) an…

天体物理学 · 物理学 2009-10-31 David B. Cline , Christina Matthey , Stanislaw Otwinowski

Gamma-ray bursts (GRBs) rank among the most powerful astrophysical phenomena, characterized by complex and highly variable prompt emission light curves that reflect the dynamics of their central engines. In this work, we analyze a sample of…

高能天体物理现象 · 物理学 2026-01-28 Ruo-Yu Guan , Fei-Fei Wang , Yuan-Chuan Zou
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