Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
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arXiv
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| Hauptverfasser: | , |
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| Format: | Preprint |
| Veröffentlicht: |
2024
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| _version_ | 1866915218988204032 |
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| author | Hamil, B. Lütfüoğlu, B. C. |
| author_facet | Hamil, B. Lütfüoğlu, B. C. |
| contents | Current observations show that a significant fraction of the Universe is composed of dark energy and dark matter. In this paper, we investigate the simultaneous effects of these dark sectors on the Euler-Heisenberg black hole, using the quintessence matter field and perfect fluid to model them. In particular, we study the black hole's thermodynamics, shadows, and quasinormal modes, and discuss in detail how these properties change with relatively large or small dark sector components. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_02109 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes Hamil, B. Lütfüoğlu, B. C. General Relativity and Quantum Cosmology Current observations show that a significant fraction of the Universe is composed of dark energy and dark matter. In this paper, we investigate the simultaneous effects of these dark sectors on the Euler-Heisenberg black hole, using the quintessence matter field and perfect fluid to model them. In particular, we study the black hole's thermodynamics, shadows, and quasinormal modes, and discuss in detail how these properties change with relatively large or small dark sector components. |
| title | Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2406.02109 |