GRB Fireball Physics: Prompt and Early Emission
arXiv:astro-ph/0609173 · doi:10.1088/1367-2630/8/9/199
Abstract
We review the fireball shock model of gamma-ray burst prompt and early afterglow emission in light of rapid follow-up measurements made and enabled by the multi-wavelength Swift satellite. These observations are leading to a reappraisal and expansion of the previous standard view of the GRB and its fireball. New information on the behavior of the burst and afterglow on minutes to hour timescales has led, among other results, to the discovery and follow-up of short GRB afterglows, the opening up of the z>6 redshift range, and the first prompt multi-wavelength observations of a long GRB-supernova. We discuss the salient observational results and some associated theoretical issues.
23 pages. Published in the New Journal of Physics Focus Issue, "Focus on Gamma-Ray Bursts in the Swift Era" (Eds. D. H. Hartmann, C. D. Dermer & J. Greiner). V2: Minor changes
References in corpus (2)
Cited by in corpus (5)
- Phase transitions and He-synthesis driven winds in neutrino cooled accretion disks: prospects for late flares in short gamma-ray bursts
- Prompt GeV-TeV Emission of Gamma-Ray Bursts Due to High-Energy Protons, Muons and Electron-Positron Pairs
- The short GRB070707 afterglow and its very faint host galaxy
- Some Theoretical Implications of Short-Hard Gamma-Ray Burst observations
- Relationship between pulse width and energy in GRB 060124: from X-ray to gamma-ray bands