Einstein constraints: Uniqueness and nonuniqueness in the conformal thin sandwich approach
- 1. Department of Physics and Astronomy, Bowdoin College, Brunswick, Maine 04011 (United States)
- 2. Physics Department, University College, Cork (Ireland)
- 3. Theoretical Astrophysics, California Institute of Technology, Pasadena, California 91125 (United States)
Description
We study the appearance of multiple solutions to certain decompositions of Einstein's constraint equations. Pfeiffer and York recently reported the existence of two branches of solutions for a particular family of background data in the extended conformal thin-sandwich decomposition. We show that the Hamiltonian constraint alone, when expressed in a certain way, admits two branches of solutions with properties very similar to those found by Pfeiffer and York. We construct these two branches analytically for a constant-density star in spherical symmetry, but argue that this behavior is more general. In the case of the Hamiltonian constraint this nonuniqueness is well known to be related to the sign of one particular term, and we argue that the extended conformal thin-sandwich equations contain a similar term that causes the breakdown of uniqueness
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.75.044009;
- arXiv
- arXiv:gr-qc/0610120v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 75
- Journal Issue
- 4
- Journal Page Range
- p. 044009-044009.9
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39033363
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- COSMOLOGICAL MODELS; COSMOLOGY; HAMILTONIANS; MATHEMATICAL SOLUTIONS; SPHERICAL CONFIGURATION; SYMMETRY
- Descriptors DEC
- CONFIGURATION; MATHEMATICAL MODELS; MATHEMATICAL OPERATORS; QUANTUM OPERATORS
Optional Information
- Notes
- (c) 2007 The American Physical Society