Spherical Fallback Accretion -the Engine GRB 050502B
| dc.contributor.advisor | Wetro, Legesse (PhD) | |
| dc.contributor.author | Misganaw, Mekdes | |
| dc.date.accessioned | 2018-06-28T12:36:59Z | |
| dc.date.accessioned | 2023-11-09T11:23:59Z | |
| dc.date.available | 2018-06-28T12:36:59Z | |
| dc.date.available | 2023-11-09T11:23:59Z | |
| dc.date.issued | 2016-09 | |
| dc.description.abstract | Gamma ray bursts are energetic and most luminous objects in the universe. They emit the most energetic form of electromagnetic radiation with extremely short wavelength and high frequencies. The gamma ray burst which is detected by swift Burst Alert Telescope (BAT) with giant and bright are is GRB 050502B with the energy band (0.3 - 10.0 keV). In this thesis we have tried to theoretically reconstruct the X-ray after-glow from GRB 050502B as observed by NASA`s Swift satellite based on current GRB model | en_US |
| dc.identifier.uri | http://10.90.10.223:4000/handle/123456789/4690 | |
| dc.language.iso | en | en_US |
| dc.publisher | Addis Ababa University | en_US |
| dc.subject | Spherical Fallback Accretion | en_US |
| dc.title | Spherical Fallback Accretion -the Engine GRB 050502B | en_US |
| dc.type | Thesis | en_US |