A theoretical study of different zone formation in fermi bubbles
| dc.contributor.author | MUHAMMAD ARIF | |
| dc.date.accessioned | 2025-11-18T12:40:34Z | |
| dc.date.available | 2025-11-18T12:40:34Z | |
| dc.date.issued | 2023 | |
| dc.description.abstract | Fermi bubbles are formed by the release of large amount of energy from the black holes by tidal disruption at the center of galaxy. We divide these fermi bubbles into different regions. These regions include strong gravitational potential zone, a cumulative zone of diffusive, non-diffusive, and thermal region. While the last one is quasi-thermal zone. We study energy transfer mechanism by the irregularities produced by magnetic fluctuations in these regions. | |
| dc.identifier.uri | https://escholar.umt.edu.pk/handle/123456789/10553 | |
| dc.language.iso | en | |
| dc.publisher | UMT, Lahore | |
| dc.title | A theoretical study of different zone formation in fermi bubbles | |
| dc.type | Thesis |
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