Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT

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dc.contributor.author Bhattacharyya, Arpan
dc.contributor.author Ghosh, Debodirna
dc.contributor.author Ghosh, Saptaswa
dc.contributor.author Pal, Sounak
dc.coverage.spatial United States of America
dc.date.accessioned 2024-07-18T09:08:29Z
dc.date.available 2024-07-18T09:08:29Z
dc.date.issued 2024-07
dc.identifier.citation Bhattacharyya, Arpan; Ghosh, Debodirna; Ghosh, Saptaswa and Pal, Sounak, "Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT", arXiv, Cornell University Library, DOI: arXiv:2407.07195, Jul. 2024.
dc.identifier.uri http://arxiv.org/abs/2407.07195
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/10248
dc.description.abstract 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.
dc.description.statementofresponsibility by Arpan Bhattacharyya, Debodirna Ghosh, Saptaswa Ghosh and Sounak Pal
dc.language.iso en_US
dc.publisher Cornell University Library
dc.title Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT
dc.type Article
dc.relation.journal arXiv


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