Choked accretion onto Kerr-Sen black holes in Einstein-Maxwell-dilaton-axion gravity
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arXiv
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| Hauptverfasser: | , , , |
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| Format: | Preprint |
| Veröffentlicht: |
2023
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| _version_ | 1866911796624883712 |
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| author | Feng, Haiyuan Wu, Yingdong Yang, Rong-Jia Modesto, Leonardo |
| author_facet | Feng, Haiyuan Wu, Yingdong Yang, Rong-Jia Modesto, Leonardo |
| contents | We investigate the process of an ultrarelativistic fluid accreted onto axisymmetric Kerr-Sen black holes in Einstein-Maxwell-dilaton-axion theory. We obtain the solution describing the velocity potential of a stationary irrotational fluid with a stiff equation of state and the solution for the streamlined diagram of the quadrupolar flow. We also investigate how the solution's coefficients and the stagnation points are affected by the parameters. The injection rate, the ejection rate, and the critical angle are discussed in detail. We find that with an increasing dilaton parameter the ratio of the ejection rate to the injection rate increases and that the radiative efficiency is larger, while the redshift is lower, compared to the Kerr black hole. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2301_02779 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Choked accretion onto Kerr-Sen black holes in Einstein-Maxwell-dilaton-axion gravity Feng, Haiyuan Wu, Yingdong Yang, Rong-Jia Modesto, Leonardo High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology We investigate the process of an ultrarelativistic fluid accreted onto axisymmetric Kerr-Sen black holes in Einstein-Maxwell-dilaton-axion theory. We obtain the solution describing the velocity potential of a stationary irrotational fluid with a stiff equation of state and the solution for the streamlined diagram of the quadrupolar flow. We also investigate how the solution's coefficients and the stagnation points are affected by the parameters. The injection rate, the ejection rate, and the critical angle are discussed in detail. We find that with an increasing dilaton parameter the ratio of the ejection rate to the injection rate increases and that the radiative efficiency is larger, while the redshift is lower, compared to the Kerr black hole. |
| title | Choked accretion onto Kerr-Sen black holes in Einstein-Maxwell-dilaton-axion gravity |
| topic | High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2301.02779 |