Physical parameters of the relativistic shock waves in GRBs: The case of 30 GRBs

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DC Field	Value	Language
dc.rights.license	BY-NC-ND	-
dc.contributor.author	Simić, Saša	-
dc.contributor.author	Popović L.	-
dc.date.accessioned	2020-09-19T18:41:40Z	-
dc.date.available	2020-09-19T18:41:40Z	-
dc.date.issued	2012	-
dc.identifier.issn	0218-2718	-
dc.identifier.uri	https://scidar.kg.ac.rs/handle/123456789/9607	-
dc.description.abstract	Using the modified internal shock wave model, we fit the gamma ray burst (GRB) light and spectral curves of 30 GRBs observed with BATSE. From the best fitting, we obtain basic parameters of the relativistic shells which are in good agreement with predictions given earlier. We compare measured GRB parameters with those obtained from the model and discuss connections between them in the frame of the physical processes laying behind GRB events. © 2012 World Scientific Publishing Company.	-
dc.rights	openAccess	-
dc.rights.uri	https://creativecommons.org/licenses/by-nc-nd/4.0/	-
dc.source	International Journal of Modern Physics D	-
dc.title	Physical parameters of the relativistic shock waves in GRBs: The case of 30 GRBs	-
dc.type	article	-
dc.identifier.doi	10.1142/S0218271812500289	-
dc.identifier.scopus	2-s2.0-84859736952	-
Appears in Collections:	Faculty of Science, Kragujevac

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