Abstract
I review some key observables seen during gamma-ray bursts (GRB) prompt emission phase. These include: the narrow distribution of the peak energy at the sub-MeV range, the peak energy - luminosity relation and the clustering of the low energy spectral slope index around 〈α〉 ∼ −1. I confront the different theoretical suggestions with these observations, discussing: (1) optically thin emission models; (2) pure ”Planck”spectra; (3) broadened ”Planck” spectra, caused by (a) sub-photospheric heating, and (b) geometrical broadening. I discuss the success and failure of each of these models in explaining the observed spectra.
Original language | English |
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Title of host publication | On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories |
Editors | Robert T. Jantzen, Kjell Rosquist, Remo Ruffini, Remo Ruffini |
Publisher | World Scientific |
Pages | 1765-1767 |
Number of pages | 3 |
ISBN (Print) | 9789814612142 |
DOIs | |
State | Published - 2015 |
Externally published | Yes |
Event | 13th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, MG13 2012 - Stockholm, Sweden Duration: 1 Jul 2015 → 7 Jul 2015 |
Publication series
Name | The 13th Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories - Proceedings of the MG13 Meeting on General Relativity, 2012 |
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Volume | 0 |
Conference
Conference | 13th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation, and Relativistic Field Theories, MG13 2012 |
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Country/Territory | Sweden |
City | Stockholm |
Period | 1/07/15 → 7/07/15 |
Bibliographical note
Publisher Copyright:© 2015, World Scientific. All rights reserved.
Keywords
- Gamma-rays: bursts
- Radiation mecha-nism: thermal
- Radiation mechanism: non-thermal