Computer Science – Sound
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1133..288d&link_type=abstract
GAMMA-RAY BURST: Sixth Huntsville Symposium. AIP Conference Proceedings, Volume 1133, pp. 288-293 (2009).
Computer Science
Sound
Gamma-Ray Sources, Gamma-Ray Bursts, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Macrosonic Propagation, Finite Amplitude Sound, Shock Waves
Scientific paper
We compute the emission from internal shocks using a new approach, where a detailed model for the dynamics of shock waves is coupled to a radiative code that solves the time evolution of shock-accelerated electrons and emitted photons in the comoving frame of the shocked material, taking into account all relevant radiative processes. Using this model, we discuss which process (synchrotron vs inverse Compton) is most likely dominating the observed low gamma-ray emission and consider a possible mechanism to reconcile the synchrotron process with the observed spectral slope (α~-1) in this energy range. We then focus on the high-energy emission (Fermi-LKT range) and show that very different spectral shapes can be expected. We describe physical diagnostics to constrain the properties of the relativistic outflow, the physical conditions in the shocked medium and the dominant radiative process.
Bošnjak Željka
Daigne Frederic
Dubus Guillaume
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