Well-posed constrained evolution of 3+1 formulations of general relativity

Vasileios Paschalidis, Alexei Khokhlov, and Igor Novikov
Phys. Rev. D 75, 024026 – Published 19 January 2007

Abstract

We present an analysis of well-posedness of constrained evolution of 3+1 formulations of general relativity. In this analysis we explicitly take into account the energy and momentum constraints as well as possible algebraic constraints on the evolution of high-frequency perturbations of solutions of Einstein’s equations. In this respect, our approach is principally different from standard analyses of well-posedness of free evolution in general relativity. Our study reveals the existence of subsets of the linearized Einstein’s equations that control the well-posedness of constrained evolution. It is demonstrated that the well-posedness of Arnowitt-Deser-Misner (ADM), Baumgarte-Shapiro-Shibata-Nakamura and other 3+1 formulations derived from the ADM formulation by adding combinations of constraints to the right-hand side of the ADM formulation and/or by linear transformation of the dynamical ADM variables depends entirely on the properties of the gauge. For certain classes of gauges we formulate conditions for well-posedness of constrained evolution. This provides a new basis for constructing stable numerical integration schemes for a classical ADM and many other 3+1 formulations of general relativity.

  • Received 19 November 2005

DOI:https://doi.org/10.1103/PhysRevD.75.024026

©2007 American Physical Society

Authors & Affiliations

Vasileios Paschalidis1, Alexei Khokhlov1,2, and Igor Novikov2,3,4

  • 1Department of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA
  • 2Enrico Fermi Institute, The University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA
  • 3Niels Bohr Institute, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
  • 4Astro Space Center of P.N. Lebedev Physical Institute, Profsoyuznaya 84/32, Moscow, 117810, Russia

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Issue

Vol. 75, Iss. 2 — 15 January 2007

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