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http://hdl.handle.net/2289/1346| Title: | Flat spectrum gamma ray burst afterglows |
| Authors: | Bhattacharya, D. |
| Keywords: | Gamma Ray Burst Afterglow Radiation Mechanism Theory |
| Issue Date: | Jun-2001 |
| Publisher: | The Astronomical Society of India |
| Citation: | Bulletin of the Astronomical Society of India, 2001, Vol.29, p107-114 |
| 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. |
| URI: | http://hdl.handle.net/2289/1346 |
| ISSN: | 0304-9523 |
| Alternative Location: | http://adsabs.harvard.edu/cgi-bin/bib_query?2001BASI...29..107B |
| Copyright: | (2001) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System. |
| Appears in Collections: | Research Papers (A&A) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 2001.BASI.29.P107.pdf | 8p. | 604.62 kB | Adobe PDF | View/Open |
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