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

A bstract 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.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-04-23
DOI
https://doi.org/10.1007/jhep04(2025)175
Citations
8
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
9.24
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article

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

Sounak Pal, Arpan Bhattacharyya, Debodirna Ghosh, Saptaswa Ghosh
8 citations
Journal of High Energy Physics
Pulsars and Gravitational Waves Research
9.24
article

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

Sounak Pal, Arpan Bhattacharyya, Debodirna Ghosh, Saptaswa Ghosh
article en
8 citations

Abstract

A bstract 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.

Journal of High Energy PhysicsVol. 2025(4)
Saha Institute of Nuclear Physics (IN), Homi Bhabha National Institute (IN), Indian Institute of Technology Gandhinagar (IN)
Openalex Percentile: Top 2%
Pulsars and Gravitational Waves Research
9.24
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