Dynamical Implications of the Kerr Multipole Moments for Spinning Black Holes
Trevor Scheopner, Justin Vines

TL;DR
This paper explores how the Kerr black hole's multipole moments determine gravitational couplings and affect scattering amplitudes, providing new insights into the structure of spinning black holes and their interactions.
Contribution
It establishes that Kerr solutions uniquely determine all multipole moments and related couplings, and derives all-order expressions for Compton amplitudes of spinning bodies.
Findings
All multipole moments of Kerr black holes are fixed by the solution.
Additional couplings do not affect three-point amplitudes but influence Compton scattering.
Explicit expressions for electromagnetic and gravitational Compton amplitudes are provided.
Abstract
Previously the linearized stress tensor of a stationary Kerr black hole has been used to determine some of the values of gravitational couplings for a spinning black hole to linear order in the Riemann tensor in the action (worldline or quantum field theory). In particular, the couplings on operators containing derivative structures of the form acting on the Riemann tensor were fixed, with the spin vector of the black hole. In this paper we find that the Kerr solution determines all of the multipole moments in the sense of Dixon of a stationary spinning black hole and that these multipole moments determine all linear in couplings. For example, additional couplings beyond the previously mentioned are fixed on operators containing derivative structures of the form acting on the Riemann tensor with the momentum vector of…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Experimental and Theoretical Physics Studies
