Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2403.14596 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866913994077372416 |
|---|---|
| author | Fernandes, Pedro G. S. Burrage, Clare Eichhorn, Astrid Sotiriou, Thomas P. |
| author_facet | Fernandes, Pedro G. S. Burrage, Clare Eichhorn, Astrid Sotiriou, Thomas P. |
| contents | In this work, we explore the properties and shadows of spin-induced scalarized black holes, as well as investigate how a Ricci coupling influences them. Our findings reveal significant deviations from the Kerr metric in terms of the location and geodesic frequencies of the innermost stable circular orbit and light ring, with the former exhibiting more pronounced disparities. The shadows of scalarized black holes exhibit relatively minor deviations when compared to those of Kerr black holes with the same mass and spin. Overall, the presence of a Ricci coupling is observed to mitigate deviations from the Kerr metric. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_14596 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Shadows and Properties of Spin-Induced Scalarized Black Holes with and without a Ricci Coupling Fernandes, Pedro G. S. Burrage, Clare Eichhorn, Astrid Sotiriou, Thomas P. General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena High Energy Physics - Theory In this work, we explore the properties and shadows of spin-induced scalarized black holes, as well as investigate how a Ricci coupling influences them. Our findings reveal significant deviations from the Kerr metric in terms of the location and geodesic frequencies of the innermost stable circular orbit and light ring, with the former exhibiting more pronounced disparities. The shadows of scalarized black holes exhibit relatively minor deviations when compared to those of Kerr black holes with the same mass and spin. Overall, the presence of a Ricci coupling is observed to mitigate deviations from the Kerr metric. |
| title | Shadows and Properties of Spin-Induced Scalarized Black Holes with and without a Ricci Coupling |
| topic | General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena High Energy Physics - Theory |
| url | https://arxiv.org/abs/2403.14596 |