Spin-induced Scalarized Black Holes in Einstein-Maxwell-scalar Models
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arXiv
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| Autori principali: | , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866912445844422656 |
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| author | Cheng, Lang Guo, Guangzhou Wang, Peng Yang, Haitang |
| author_facet | Cheng, Lang Guo, Guangzhou Wang, Peng Yang, Haitang |
| contents | We construct spin-induced scalarized black hole solutions in a class of Einstein-Maxwell-scalar models, where a scalar field is non-minimally coupled to the electromagnetic field. Our results show that scalar hair develops only for rapidly rotating black holes, while slowly spinning ones remain well described by the Kerr-Newman (KN) metric. The scalar field contributes only a small fraction of the total mass, indicating suppressed nonlinear effects. This suppression may account for the narrow existence domains of scalarized black holes and the similarities observed in their existence domains across different coupling functions. Moreover, scalarized black holes are found to coexist with linearly stable, entropically favored KN black holes. These results motivate further investigations into the nonlinear dynamics and stability of scalarized black holes in these models. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2506_01773 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Spin-induced Scalarized Black Holes in Einstein-Maxwell-scalar Models Cheng, Lang Guo, Guangzhou Wang, Peng Yang, Haitang General Relativity and Quantum Cosmology We construct spin-induced scalarized black hole solutions in a class of Einstein-Maxwell-scalar models, where a scalar field is non-minimally coupled to the electromagnetic field. Our results show that scalar hair develops only for rapidly rotating black holes, while slowly spinning ones remain well described by the Kerr-Newman (KN) metric. The scalar field contributes only a small fraction of the total mass, indicating suppressed nonlinear effects. This suppression may account for the narrow existence domains of scalarized black holes and the similarities observed in their existence domains across different coupling functions. Moreover, scalarized black holes are found to coexist with linearly stable, entropically favored KN black holes. These results motivate further investigations into the nonlinear dynamics and stability of scalarized black holes in these models. |
| title | Spin-induced Scalarized Black Holes in Einstein-Maxwell-scalar Models |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2506.01773 |