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If gamma ray bursts are highly collimated, the energy requirements of each event may be reduced by several (~ 4-6) orders of magnitude, and the event rate increased correspondingly. Extreme conditions in gamma ray bursters lead to highly…

天体物理学 · 物理学 2009-10-30 James E. Rhoads

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…

天体物理学 · 物理学 2009-11-10 Weiqun Zhang , S. E. Woosley , A. Heger

We have studied the relativistic beamed outflow proposed to occur in the collapsar model of gamma-ray bursts. A jet forms as a consequence of an assumed energy deposition of $\sim 10^{50}- 10^{51}$ erg/s within a $30^{\circ}$ cone around…

天体物理学 · 物理学 2007-05-23 Miguel A. Aloy , Ewald Mueller , Jose M. Ibanez , Jose M. Marti , Andrew MacFadyen

The intrinsic luminosity functions of extremely fast jets found in many active galaxies and gamma-ray bursts are difficult to measure since their apparent luminosities are strongly affected by relativistic beaming. Past studies have only…

天体物理学 · 物理学 2009-11-10 Matthew L. Lister

We study the effects of the beaming-induced luminosity function on statistics of observed GRBs, assuming the cosmological scenario. We select and divide the BATSE 4B data into 588 long bursts (T$_{90}>2.5$ sec) and 149 short bursts…

天体物理学 · 物理学 2009-10-31 Chunglee Kim , Heon-Young Chang , Insu Yi

Knowledge of the bulk Lorentz factor $\Gamma_{0}$ of GRBs allows us to compute their comoving frame properties shedding light on their physics. Upon collisions with the circumburst matter, the fireball of a GRB starts to decelerate,…

高能天体物理现象 · 物理学 2018-01-31 G. Ghirlanda , F. Nappo , G. Ghisellini , A. Melandri , G. Marcarini , L. Nava , O. S. Salafia , S. Campana , R. Salvaterra

Motivated by GW170817 we examine constraints that observations put on the angular structure of long gamma-ray burst (GRB) jets. First, the relatively narrow observed distribution of $E_{X}/E_{\gamma}$ (the isotropic equivalent early X-ray…

高能天体物理现象 · 物理学 2018-12-12 Paz Beniamini , Ehud Nakar

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA…

宇宙学与河外天体物理 · 物理学 2014-11-20 T. Savolainen , D. C. Homan , T. Hovatta , M. Kadler , Y. Y. Kovalev , M. L. Lister , E. Ros , J. A. Zensus

The distribution of the apparent total energy emitted by a gamma-ray burst reflects not only the distribution of the energy actually released by the burst engine, but also the distribution of beaming angles. Using the observed energy…

天体物理学 · 物理学 2009-11-06 David L. Band

Gamma-ray bursts are believed to be some catastrophic event in which material is ejected at a relativistic velocity, and internal collisions within this ejecta produce the observed $\gamma$-ray flash. The angular size of a causally…

天体物理学 · 物理学 2009-10-31 Pawan Kumar , Tsvi Piran

We present numerical solutions of the 2D relativistic hydrodynamics equations describing the deceleration and expansion of highly relativistic conical jets, of opening angles 0.05<theta<0.2, propagating into a medium of uniform density. Jet…

高能天体物理现象 · 物理学 2015-05-27 N. Wygoda , E. Waxman , D. Frail

There exists an inevitable scatter in intrinsic luminosity of Gamma Ray Bursts(GRBs). If there is relativistic beaming in the source, viewing angle variation necessarily introduces variation in the intrinsic luminosity function(ILF).…

高能天体物理现象 · 物理学 2022-03-23 Shreya Banerjee , David Eichler , Dafne Guetta

The early X-ray afterglow for a significant number of gamma-ray bursts detected by the Swift satellite is observed to have a phase of very slow flux decline with time ($F_\nu \propto t^{-\alpha}$ with $0.2 \lesssim \alpha \lesssim 0.8$) for…

天体物理学 · 物理学 2009-11-13 Jonathan Granot , Pawan Kumar

The observed apparent velocities and luminosities of the relativistic jets in AGNs are significantly different from their intrinsic values due to strong special relativistic effects. We adopt the maximum likelihood method to determine…

天体物理学 · 物理学 2009-11-13 Yuan Liu , Shuang Nan Zhang

The fate and observable properties of gamma-ray burst jets depend crucially on their interaction with the progenitor material that surrounds the central engine. We present a semi-analytical model of such interaction, which builds upon…

高能天体物理现象 · 物理学 2020-04-29 O. S. Salafia , C. Barbieri , S. Ascenzi , M. Toffano

We construct models for gamma-ray bursts where the emission comes from internal shocks in a relativistic wind with a highly non uniform distribution of the Lorentz factor. We follow the evolution of the wind using a very simplified approach…

天体物理学 · 物理学 2009-10-30 F. Daigne , R. Mochkovitch

The variety of gamma-ray burst phenomenology could be largely attributable to differences in the opening angle of an isotropic outflow or to a standard type of event viewed from different orientations. Motivated by this currently popular…

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

We present a model for relativistic jets which generates a particular angular distribution of Lorentz factor and energy per solid angle. We consider a fireball with specific internal energy E/M launched with bulk Lorentz factor \gamma_B.…

高能天体物理现象 · 物理学 2015-06-16 Paul C. Duffell , Andrew I. MacFadyen

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

The low energy spectra of some gamma-ray bursts' show excess components beside the power-law dependence. The consequences of such a feature allows to estimate the gamma photometric redshift of the long gamma-ray bursts in the BATSE Catalog.…

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