Flat spectrum gamma ray burst afterglows
| dc.contributor.author | Bhattacharya, D | |
| dc.date.accessioned | 2006-06-12T06:43:40Z | |
| dc.date.available | 2006-06-12T06:43:40Z | |
| dc.date.issued | 2001-06 | |
| dc.description.abstract | Temporal behaviour of GRB afterglow light curve is derived for the case where the electron energy distribution is relatively hard, with the power-law index p lying between 1.0 and 2.0. It is shown that the expected behaviour will be the same as that for p > 2.0 if the upper cutoff in the electron energy distribution evolves in direct proportion to the bulk Lorentz factor of the blast wave. | en |
| dc.format.extent | 619131 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Bulletin of the Astronomical Society of India, 2001, Vol.29, p107-114 | en |
| dc.identifier.issn | 0304-9523 | |
| dc.identifier.uri | http://hdl.handle.net/2289/1346 | |
| dc.language.iso | en | en |
| dc.publisher | The Astronomical Society of India | en |
| dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?2001BASI...29..107B | en |
| dc.rights | (2001) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System. | en |
| dc.subject | Gamma Ray Burst | en |
| dc.subject | Afterglow | en |
| dc.subject | Radiation Mechanism | en |
| dc.subject | Theory | en |
| dc.title | Flat spectrum gamma ray burst afterglows | en |
| dc.type | Article | en |