An Observed Correlation Between Thermal and Non-Thermal Emission in Gamma-Ray Bursts
arXiv:1403.0374 · doi:10.1088/2041-8205/784/2/L43
Abstract
Recent observations by the Gamma-ray Space Telescope have confirmed the existence of thermal and non-thermal components in the prompt photon spectra of some Gamma-ray bursts (GRBs). Through an analysis of six bright Fermi GRBs, we have discovered a correlation between the observed photospheric and non-thermal -ray emission components of several GRBs using a physical model that has previously been shown to be a good fit to the Fermi data. From the spectral parameters of these fits we find that the characteristic energies, and , of these two components are correlated via the relation which varies from GRB to GRB. We present an interpretation in which the value of index indicates whether the jet is dominated by kinetic or magnetic energy. To date, this jet composition parameter has been assumed in the modeling of GRB outflows rather than derived from the data.
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Cited by in corpus (12)
- The Physics of Gamma-Ray Bursts and Relativistic Jets
- The Fermi GBM Gamma-Ray Burst Spectral Catalog: 10 Years of Data
- Photosphere emission in the X-Ray Flares of Swift Gamma-Ray Bursts and Implications for the Fireball Properties
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- Ultra-high Energy Cosmic Rays and Neutrinos from Gamma-Ray Bursts, Hypernovae and Galactic Shocks
- Testing a model for subphotospheric dissipation in GRBs: fits to Fermi data constrain the dissipation scenario
- Constraining the bulk Lorentz factor from the photosphere emission
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