Linear instability of nonvacuum spacetimes

David Kastor and Jennie Traschen
Phys. Rev. D 47, 480 – Published 15 January 1993
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Abstract

We study the problem of linear instability in nonvacuum spacetimes. For vacuum spacetimes linear instability occurs when the spacetime has Killing vectors. In the nonvacuum case, one must prescribe how the sources are to vary. For one natural choice, we show that the signal for instability is the existence of integral constraint vector fields. These vector fields lead, as in the vacuum case, to nonlinear constraints on the first-order perturbations to the metric and momentum. For other choices for variations of the sources, we show how to modify the definition of integral constraint vectors appropriately. Since Robertson-Walker spacetimes have integral constraint vectors our results may have cosmological applications.

  • Received 30 September 1991

DOI:https://doi.org/10.1103/PhysRevD.47.480

©1993 American Physical Society

Authors & Affiliations

David Kastor

  • Stanford Linear Accelerator Center, Stanford University, Stanford, California 94305

Jennie Traschen

  • Department of Physics and Astronomy, University of Massachusetts, Amherst, Massachusetts 01003

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Vol. 47, Iss. 2 — 15 January 1993

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