Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT
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arXiv
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| Autores principales: | , , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866915254311583744 |
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| author | Bhattacharyya, Arpan Ghosh, Debodirna Ghosh, Saptaswa Pal, Sounak |
| author_facet | Bhattacharyya, Arpan Ghosh, Debodirna Ghosh, Saptaswa Pal, Sounak |
| contents | In this paper, we compute the WQFT partition function, specifically the eikonal phase in a black hole scattering event in the dynamical Chern-Simons theory, using the techniques of spinning worldline quantum field theory. We consider the scattering of spinning black holes and highlight the necessary details for the calculation of the partition function. We present the $ε$-expansion of the essential two-loop integrals using Integration-by-Parts (IBP) reduction and differential equation techniques, which we then utilize to compute the linear-in-order spin eikonal phase up to 3PM. Additionally, we discuss the dependence of the phase on the spin orientations of the black holes. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_07195 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT Bhattacharyya, Arpan Ghosh, Debodirna Ghosh, Saptaswa Pal, Sounak High Energy Physics - Theory General Relativity and Quantum Cosmology High Energy Physics - Phenomenology In this paper, we compute the WQFT partition function, specifically the eikonal phase in a black hole scattering event in the dynamical Chern-Simons theory, using the techniques of spinning worldline quantum field theory. We consider the scattering of spinning black holes and highlight the necessary details for the calculation of the partition function. We present the $ε$-expansion of the essential two-loop integrals using Integration-by-Parts (IBP) reduction and differential equation techniques, which we then utilize to compute the linear-in-order spin eikonal phase up to 3PM. Additionally, we discuss the dependence of the phase on the spin orientations of the black holes. |
| title | Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT |
| topic | High Energy Physics - Theory General Relativity and Quantum Cosmology High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2407.07195 |