Gravitational losses for the binary systems induced by the next-to-leading spin-orbit coupling effects
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arXiv
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| Autores principales: | , , , , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| Materias: | |
| Acceso en línea: | |
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| _version_ | 1866907785925492736 |
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| author | Zhang, Hao Gao, Wei He, Guansheng Liu, Siming Jia, Huanyu Lin, Wenbin |
| author_facet | Zhang, Hao Gao, Wei He, Guansheng Liu, Siming Jia, Huanyu Lin, Wenbin |
| contents | The orbital energy and momentum of the compact binary systems will loss due to gravitational radiation. Based on the mass and mass-current multipole moments of the binary system with the spin vector defined by Bohé et al. [Class. Quantum Grav. 30, 075017 (2013)], we calculate the loss rates of energy, angular and linear momentum induced by the next-to-leading spin-orbit effects. For the case of circular orbit, the formulations for these losses are given in terms of the orbital frequency. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2402_02170 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Gravitational losses for the binary systems induced by the next-to-leading spin-orbit coupling effects Zhang, Hao Gao, Wei He, Guansheng Liu, Siming Jia, Huanyu Lin, Wenbin General Relativity and Quantum Cosmology The orbital energy and momentum of the compact binary systems will loss due to gravitational radiation. Based on the mass and mass-current multipole moments of the binary system with the spin vector defined by Bohé et al. [Class. Quantum Grav. 30, 075017 (2013)], we calculate the loss rates of energy, angular and linear momentum induced by the next-to-leading spin-orbit effects. For the case of circular orbit, the formulations for these losses are given in terms of the orbital frequency. |
| title | Gravitational losses for the binary systems induced by the next-to-leading spin-orbit coupling effects |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2402.02170 |