Quasistationary binary inspiral. I. Einstein equations for the two Killing vector spacetime

John T. Whelan and Joseph D. Romano
Phys. Rev. D 60, 084009 – Published 17 September 1999
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Abstract

The inspiral of a binary system of compact objects due to gravitational radiation is investigated using the toy model of two infinitely long lines of mass moving in a fixed circular orbit. The two Killing fields in the toy model are used, according to a formalism introduced by Geroch, to describe the geometry entirely in terms of a set of tensor fields on the two-manifold of Killing vector orbits. Geroch’s derivation of the Einstein equations in this formalism is streamlined and generalized. The explicit Einstein equations for the toy model spacetime are derived in terms of the degrees of freedom which remain after a particular choice of gauge.

  • Received 14 April 1999

DOI:https://doi.org/10.1103/PhysRevD.60.084009

©1999 American Physical Society

Authors & Affiliations

John T. Whelan*

  • Institut für Theoretische Physik, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland

Joseph D. Romano

  • Department of Physical Sciences, University of Texas at Brownsville, Brownsville, Texas 78521

  • *Electronic address: whelan@itp.unibe.ch
  • Electronic address: jromano@utb1.utb.edu

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Vol. 60, Iss. 8 — 15 October 1999

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