corner
corner

Phys. Rev. D 75, 024026 (2007) [20 pages]

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

Download: PDF (288 kB) Buy this article Export: BibTeX or EndNote (RIS)

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

Received 19 November 2005; published 19 January 2007

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.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.75.024026
DOI:
10.1103/PhysRevD.75.024026
PACS:
04.25.Dm, 04.70.Bw