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Extremely hard GRB spectra prune down the forest of emission models

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In this article, the authors consider the evidence for very hard low energy spectra during the prompt phase of Gamma-Ray Bursts (GRB), and examine the spectral evolution of GRB 980306 together with the detailed analysis of some other bursts already presented in the literature.
Abstract
We consider the evidence for very hard low energy spectra during the prompt phase of Gamma-Ray Bursts (GRB). In particular we examine the spectral evolution of GRB 980306 together with the detailed analysis of some other bursts already presented in the literature (GRB 911118, GRB 910807, GRB 910927 and GRB 970111), and check for the significance of their hardness (i.e. extremely steep spectral slopes below the EFE peak) by applying dierent tests. These bursts, detected by the Burst And Transient Source Experiment (BATSE) in the30 keV-2 MeV energy range, are suciently bright to allow time resolved spectral studies on time intervals of the order of tenths of a second. We discuss the hard spectra of these bursts and their evolution in the context of several non-thermal emission models, which all appear inadequate to account for these cases. The extremely hard spectra, which are detected in the early part of the BATSE light curve, are also compared with a black body spectral model: the resulting fits are remarkably good, except for an excess at high energies (in several cases) which could be simply accounted for by the presence of a supra-thermal component. The findings on the possible thermal character of the evolving spectrum and the implications on the GRB physical scenario are considered in the frameworks of photospheric models for a fireball which is becoming optically thin, and of Compton drag models, in which the fireball boosts "ambient" seed photons by its own bulk motion. Both models, according to simple estimates, appear to be qualitatively and quantitatively consistent with the found spectral characteristics, although their possible caveats are discussed.

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Journal ArticleDOI

Gamma-Ray Bursts: Progress, Problems & Prospects

TL;DR: The cosmological gamma-ray burst (GRB) phenomenon is reviewed in this article, where broad observational facts and empirical phenomenological relations of the GRB prompt emission and afterglow are outlined.
Journal ArticleDOI

General relativistic magnetohydrodynamic simulations of the jet formation and large-scale propagation from black hole accretion systems

TL;DR: In this article, the formation and large-scale propagation of Poynting-dominated jets produced by accreting, rapidly rotating black hole systems are studied by numerically integrating the general relativistic magnetohydrodynamic equations of motion to follow the self-consistent interaction between accretion discs and black holes.
Journal ArticleDOI

The Ep,i - Eiso correlation in GRBs: updated observational status, re-analysis and main implications

Lorenzo Amati
- 24 Jan 2006 - 
TL;DR: In this paper, the authors provide an update and a re-analysis of the Ep,i - Eiso correlation based on an updated sample consisting of 41 long GRBs/XRFs with firm estimates of z and observed peak energy, Ep,obs, 12 GRBs with uncertain valeus of z, 2 short GRBs, and the peculiar sub-energetic events GRB980425/SN1998bw and GRB031203/SN2003lw.
Journal ArticleDOI

The Ep,i–Eiso correlation in gamma-ray bursts: updated observational status, re-analysis and main implications

TL;DR: The E p,i -E iso correlation between the cosmological rest-frame vF v spectrum peak energy and the isotropic-equivalent radiated energy, E iso, discovered by Amati et al. as discussed by the authors, is one of the most intriguing and debated observational evidences in gamma-ray burst (GRB) astrophysics.
Journal ArticleDOI

Collisional mechanism for gamma‐ray burst emission

TL;DR: In this paper, the nuclear and Coulomb collisions in gamma-ray burst (GRB) jets create a hot e ± plasma, which radiates its energy, and a large fraction of the jet energy is converted to escaping radiation.
References
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