منابع مشابه
Prompt Neutrino Emission from Gamma-Ray Bursts
Recent observations show that some or possibly all long-duration gamma-ray bursts (GRBs) arise from the core collapse of massive stars. In this case, the GRB environments are believed to be preburst stellar winds. We here study prompt neutrino emission from reverse shocks as a result of the interaction of relativistic fireballs with their surrounding wind matter. We find that for reasonable par...
متن کاملPrompt Optical Emission from Gamma-ray Bursts
University of Michigan, Ann Arbor, MI 48109, USA Los Alamos National Laboratory, Los Alamos, NM 87545, USA NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA Universities Space Research Association, Seabrook, MD 20706, USA Raytheon Systems, Lanham, MD 20706, USA Università degli Studi di Ferrara, Ferrara, Italy Space Research Organization, Utrecht, The Netherlands Space Sciences Laborat...
متن کامل“late Prompt” Emission in Gamma Ray Bursts?
The flat decay phase in the first 10–10 seconds of the X–ray light curve of Gamma Ray Bursts (GRBs) has not yet found a convincing explanation. The fact that the optical and X–ray lightcurves are often different, with breaks at different times, makes contrived any explanation based on the same origin for both the X–ray and optical fluxes. We here assume that the central engine can be active for...
متن کاملA link between prompt optical and prompt gamma-ray emission in gamma-ray bursts.
The prompt optical emission that arrives with the gamma-rays from a cosmic gamma-ray burst (GRB) is a signature of the engine powering the burst, the properties of the ultra-relativistic ejecta of the explosion, and the ejecta's interactions with the surroundings. Until now, only GRB 990123 had been detected at optical wavelengths during the burst phase. Its prompt optical emission was variable...
متن کاملHigh Energy Emission from the Prompt Gamma-Ray Burst
We study the synchrotron and synchrotron self-Compton (SSC) emission from internal shocks that are responsible for the prompt γ-ray emission in GammaRay Bursts (GRBs), and consider the relation between these two components, taking into account the high energy cutoff due to pair production and Thomson scattering. We find that in order for the peak energy of the synchrotron to be Ep ∼ 300 keV wit...
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ژورنال
عنوان ژورنال: New Astronomy Reviews
سال: 2002
ISSN: 1387-6473
DOI: 10.1016/s1387-6473(02)00201-4