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Geometric description of lightlike foliations by an observer in general relativity

Published online by Cambridge University Press:  22 June 2005

VICENTE J. BOLÓS
Affiliation:
Dep. Matemáticas, Facultad de Ciencias, Universidad de Extremadura, Avda. de Elvas s/n. 06071-Badajoz, Spain. e-mail: vjbolos@unex.es

Abstract

We introduce new concepts and properties of lightlike distributions and foliations (of dimension and co-dimension 1) in a space-time manifold of dimension $n$, from a purely geometric point of view. Given an observer and a lightlike distribution $\Omega $ of dimension or co-dimension 1, its lightlike direction is broken down into two vector fields: a timelike vector field $U$ representing the observer and a spacelike vector field $S$ representing the relative direction of propagation of $\Omega $ for this observer. A new distribution $\Omega_U^-$ is defined, with the opposite relative direction of propagation for the observer $U$. If both distributions $\Omega $ and $\Omega_U^-$ are integrable, the pair $\{\Omega,\Omega_U^-\}$ represents the wave fronts of a stationary wave for the observer $U$. However, we show in an example that the integrability of $\Omega $ does not imply the integrability of $\Omega_U^-$.

Type
Research Article
Copyright
2005 Cambridge Philosophical Society

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