Linear-nonlinear formulation of Einstein equations for the two-body problem in general relativity

Pablo Laguna
Phys. Rev. D 60, 084012 – Published 24 September 1999
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Abstract

A formulation of Einstein equations is presented that could yield advantages in the study of collisions of binary compact objects during regimes between linear-nonlinear transitions. The key idea behind this formulation is a separation of the dynamical variables into (i) a fixed conformal 3-geometry, (ii) a conformal factor possessing nonlinear dynamics and (iii) transverse-traceless perturbations of the conformal 3-geometry.

  • Received 3 May 1999

DOI:https://doi.org/10.1103/PhysRevD.60.084012

©1999 American Physical Society

Authors & Affiliations

Pablo Laguna

  • Department of Astronomy and Astrophysics and Center for Gravitational Physics and Geometry, Penn State University, University Park, Pennsylvania 16802

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Issue

Vol. 60, Iss. 8 — 15 October 1999

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