The Causal Boundary Of Standard Stationary Spacetimes

Details The Causal Boundary Of Standard Stationary Spacetimes The Causal Boundary Of Standard Stationary Spacetimes

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1122..272f&link_type=abstract

PHYSICS AND MATHEMATICS OF GRAVITATION: Proceedings of the Spanish Relativity Meeting 2008. AIP Conference Proceedings, Volume

Mathematics

1

Field Theory, Approximation Methods, Equations Of Motion, Numerical Approximation And Analysis

Scientific paper

In this paper we present a description of the causal boundary for the class of standard stationary spacetimes: With (M,g0) an arbitrary Riemannian manifold and ω a one-form on M, the causal boundary of (V = R×M,g = -dt2+ω⊗dt+dt⊗ω+g0) is given in terms of a Busemann boundary construction on manifolds (M,F+/-), with F+/- Finsler metrics associated to ω and g0.

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