Flat Spectrum Gamma Ray Burst Afterglows
| dc.creator | Bhattacharya, Dipankar | |
| dc.date | 2001-04-15 | |
| dc.date | 2001-06-19 | |
| dc.date.accessioned | 2026-07-07T01:58:14Z | |
| dc.date.available | 2026-07-07T01:58:14Z | |
| dc.description | Temporal behaviour of GRB afterglow light curve is derived for the case where the electron energy distribution is relatively flat, 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. | |
| dc.description | 8 pages, uses basi.sty (included). Revised according to referees' comments. Added discussion on Dai & Cheng (2001) astro-ph/0105055. Accepted for publication in Bull. Astr. Soc. India | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0104250 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0104250 | |
| dc.identifier | Bull. Astr. Soc. India, vol. 29, pp. 107-114 (2001) | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2690 | |
| dc.subject | Astrophysics | |
| dc.title | Flat Spectrum Gamma Ray Burst Afterglows | |
| dc.type | text |