Testing the Kerr nature with binary black hole inspirals
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arXiv
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| Main Authors: | , , |
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| Format: | Preprint |
| Published: |
2024
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| _version_ | 1866912681603104768 |
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| author | Shashank, Swarnim Bambi, Cosimo Roy, Rittick |
| author_facet | Shashank, Swarnim Bambi, Cosimo Roy, Rittick |
| contents | The theory of general relativity (GR) is the standard framework for the description of gravitation and the geometric structure of spacetime. With the recent advancement of observational instruments, it has become possible to probe the strong field regime to test GR. We present the constraints obtained from the binary black hole inspiral data of the LIGO-Virgo-Kagra (LVK) gravitational wave (GW) observations on the deformations of some popular parametrized non-Kerr metrics. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_13798 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Testing the Kerr nature with binary black hole inspirals Shashank, Swarnim Bambi, Cosimo Roy, Rittick General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena The theory of general relativity (GR) is the standard framework for the description of gravitation and the geometric structure of spacetime. With the recent advancement of observational instruments, it has become possible to probe the strong field regime to test GR. We present the constraints obtained from the binary black hole inspiral data of the LIGO-Virgo-Kagra (LVK) gravitational wave (GW) observations on the deformations of some popular parametrized non-Kerr metrics. |
| title | Testing the Kerr nature with binary black hole inspirals |
| topic | General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2407.13798 |