Second-Order Self-Force Calculation of Gravitational Binding Energy in Compact Binaries

Adam Pound, Barry Wardell, Niels Warburton, and Jeremy Miller
Phys. Rev. Lett. 124, 021101 – Published 14 January 2020
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Abstract

Self-force theory is the leading method of modeling extreme-mass-ratio inspirals (EMRIs), key sources for the gravitational-wave detector LISA. It is well known that for an accurate EMRI model, second-order self-force effects are critical, but calculations of these effects have been beset by obstacles. In this Letter we present the first implementation of a complete scheme for second-order self-force computations, specialized to the case of quasicircular orbits about a Schwarzschild black hole. As a demonstration, we calculate the gravitational binding energy of these binaries.

  • Figure
  • Received 20 August 2019
  • Revised 10 October 2019

DOI:https://doi.org/10.1103/PhysRevLett.124.021101

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Adam Pound1, Barry Wardell2, Niels Warburton2, and Jeremy Miller1

  • 1School of Mathematical Sciences and STAG Research Centre, University of Southampton, Southampton SO17 1BJ, United Kingdom
  • 2School of Mathematics and Statistics, University College Dublin, Belfield, Dublin 4, Ireland

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Issue

Vol. 124, Iss. 2 — 17 January 2020

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