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. |
What people are saying - Write a review
We haven't found any reviews in the usual places.
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 | |
38 other sections not shown
Common terms and phrases
acceleration afterglow American analysis angle assumed band BATSE black hole break calculated component consistent correlation decay density detected detector determined Discovery discussed distribution duration E. E. Fenimore early edited effect electrons emission energy estimate et al evidence evolution expected FIGURE fireball flux function Galassi galaxy Gamma-Ray Bursts indicate initial Institute of Physics interval Italy light curve limit Lorentz factor luminosity magnetic field magnitude mass measured Nature neutrino neutron observed obtained optical outflow panel parameters peak phase photon polarization possible power-law predicted present produce prompt properties radiation range redshift REFERENCES region relation relativistic reported shock shown shows significant similar simulations spectral spectrum star structure suggest supernova synchrotron Table trigger University wave wind X-ray XRFs