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The present common view about GRB origin is related to cosmology, what is based on statistical analysis, and on measurements of the redshifts in the GRB optical afterglows of long GRB. Models of radiation, and models of the central machine…

Astrophysics · Physics 2008-11-26 G. S. Bisnovatyi-Kogan

The X-ray light curves of the early afterglow phase from gamma-ray bursts present a puzzling variability, including flares. The origin of these flares is still debated, and often associated with a late activity of the central engine. We…

High Energy Astrophysical Phenomena · Physics 2017-12-27 Astrid Lamberts , Frédéric Daigne

Based on a refined generic dynamical model, we investigate afterglows from jetted gamma-ray burst (GRB) remnants numerically. In the relativistic phase, the light curve break could marginally be seen. However, an obvious break does exist at…

Astrophysics · Physics 2016-01-27 Y. F. Huang , T. Lu , Z. G. Dai , K. S. Cheng

Gamma-ray bursts (GRBs) are one of the most exciting sources that offer valuable opportunities for investigating the evolution of energy fraction given to magnetic fields and particles through microphysical parameters during relativistic…

High Energy Astrophysical Phenomena · Physics 2023-11-07 Nissim Fraija , Maria G. Dainotti , Boris Betancourt Kamenetskaia , Antonio Galván-Gámez , Edilberto Aguilar-Ruiz

We present an analytical approach to the dynamical evolution of fireballs or axially symmetric jets expanding into an external medium, with application to Gamma-Ray Burst remnants. This method leads to numerical calculations of fireball…

Astrophysics · Physics 2016-08-30 A. Panaitescu , P. Meszaros

We use high--quality, multi-band observations of Swift GRB120404A, from gamma-ray to radio frequencies, together with the new hydrodynamics code of van Eerten et al. (2012) to test the standard synchrotron shock model. The evolution of the…

The detection of delayed emission in X-ray, optical and radio wave length, ``afterglow'', following a gamma-ray burst can be described by the emission of a relativistic shell decelerating upon collision with the ISM. We show that the…

Astrophysics · Physics 2009-10-30 Re'em Sari

Gamma-ray burst (GRB) afterglow emission is believed to be produced by synchrotron emission of electrons accelerated to high energy by a relativistic collisionless shock propagating into a weakly magnetized plasma. Afterglow observations…

Astrophysics · Physics 2010-11-11 Zhuo Li , Eli Waxman

Some progenitor models of gamma-ray bursts (GRBs) (e.g., collapsars) may produce anisotropic jets in which the energy per unit solid angle is a power-law function of the angle ($\propto\theta^{-k}$). We calculate light curves and spectra…

Astrophysics · Physics 2009-10-31 Z. G. Dai , L. J. Gou

The fireball model of gamma-ray bursts predicted that when the energetic blast wave encountered the surrounding medium, there will be afterglow emission, and the subsequent afterglow observations appeared to confirm this prediction. In this…

Astrophysics · Physics 2007-05-23 D. M. Wei , T. Lu

The detection of x-ray afterglows of gamma-ray burst (GRB) sources has enabled the optical discovery that GRBs are at cosmological distances, which confirms that the enormous luminosities required must produce a relativistically expanding…

Astrophysics · Physics 2009-10-30 Jonathan E. Grindlay

If Gamma-Ray-Bursts (GRBs) occur at high redshifts, then their bright afterglow emission can be used to probe the ionization and metal enrichment histories of the intervening intergalactic medium during the epoch of reionization. In…

Astrophysics · Physics 2009-10-31 Benedetta Ciardi , Abraham Loeb

At the time of its discovery, the optical and X-ray afterglow of GRB 970228 appeared to be a ringing endorsement of the previously untried relativistic fireball model of gamma-ray burst (GRB) afterglows, but now that nearly a dozen optical…

Astrophysics · Physics 2009-10-31 Daniel E. Reichart

We present results of model fits to afterglow data sets of GRB970508, GRB980703 and GRB070125, characterized by long and broadband coverage. The model assumes synchrotron radiation (including self-absorption) from a spherical adiabatic…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Konstantinos Leventis , Alexander J. van der Horst , Hendrik J. van Eerten , Ralph A. M. J. Wijers

Aims: Drawing an analogy with Active Galactic Nuclei, we investigate the one-zone SSC model of Gamma Ray Bursts afterglows in the presence of electron injection and cooling both by synchrotron and SSC losses. Methods: We solve the spatially…

High Energy Astrophysical Phenomena · Physics 2015-05-14 M. Petropoulou , A. Mastichiadis

Gamma-ray bursts (GRBs) show diverse X-ray afterglow light-curves, including breaks and plateaus, whose physical origins remain debated. Previous claims linked high-energy ($E \ge 100$ MeV) detection to X-ray afterglow complexity or plateau…

High Energy Astrophysical Phenomena · Physics 2026-05-27 A. A. Vigliano , F. Longo , Ž. Bošnjak

We report on BeppoSAX simultaneous X- and gamma-ray observations of the bright GRB 990123. We present the broad-band spectrum of the prompt emission, including optical, X- and gamma-rays, confirming the suggestion that the emission…

We briefly discuss the theoretical implications of recent detections of gamma-ray bursts (GRBs) by BSAX. Relativistic shock wave theories of fireball expansion are challenged by the wealth of X-ray, optical and radio data obtained after the…

Astrophysics · Physics 2009-10-30 Marco Tavani

Observations of gamma ray bursts (GRB) afterglows in different spectral bands provide a most valuable information about their nature, as well as about properties of surrounding medium. Powerful infrared afterglow was observed from the…

Astrophysics · Physics 2009-11-10 M. V. Barkov , G. S. Bisnovatyi-Kogan

We consider possible interpretations of the recently detected X- ray afterglow from the gamma-ray burst source GRB 970228. Cosmological and Galactic models of gamma-ray bursts predict different flux and spectral evolution of X-ray…

Astrophysics · Physics 2009-10-30 M. Tavani