Gamma-Ray Bursts: 30 Years of Discovery: Gamma-Ray Burst SymposiumIn the last thirty years, gamma-ray bursts have grown from an oddity to a central position in astrophysics. Not only are they the largest explosions since the big bang, capable of flooding most of the universe with gamma-rays, but their brilliance serves as a backlight that can illuminate the cosmos far deeper into the early universe than any other object. Their unpredictability has forced researchers to use extreme measures to observe them: completely autonomous satellites and robotic ground-based telescopes. Their bizarre physical properties have pushed us to develop new theories of astrophysical explosions. Topics include: global properties of GRBs; X-ray flashes; ultra-high energy gamma-rays, neutrinos, gravity waves; prompt emission and early afterglows; relativistic jets and polarization; GRB030329; GRB progenitors; GRB connection to supernovae; dark versus bright GRBs; late afterglows; GRBs and cosmology; general observations; general theory; analysis and observation techniques; present satellites; Swift satellite; future satellites; and robotic observing systems. |
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Contents
A Unified Jet Model of XRay Flashes and GammaRay Bursts | 19 |
Radiation Processes in GRBs Prompt Emission | 25 |
Broad Band 2700 keV Properties of the GRBs Observed | 31 |
Copyright | |
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afterglow American Institute analysis angle assumed background band BATSE bright calculated component consistent counts density detected detector determined Discovery distribution duration E. E. Fenimore edited effects electrons emission energy estimate et al evolution expected FIGURE fireball flux function Galassi galaxy Gamma-Ray Bursts given increase indicate initial Institute of Physics interval Italy light curve limit located Lorentz factor luminosity magnetic field magnitude measured Nature neutrino observed obtained optical parameters peak phase photon polarization position possible power-law predicted present produce prompt properties radiation range redshift REFERENCES region relation relativistic Science sensitivity shock short shown shows significant simulations Space spectral spectrum star structure supernova Swift Table telescope transient trigger University X-ray XRFs