Stability analysis of a nonscalar curvature singularity

Details Stability analysis of a nonscalar curvature singularity Stability analysis of a nonscalar curvature singularity

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..46.1424h&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 46, Issue 4, 15 August 1992, pp.1424-1428

Physics

7

Fundamental Problems And General Formalism

Scientific paper

The behavior of test scalar waves on a dust-filled type-V locally rotationally symmetric spacetime is used to probe the nonscalar curvature singularity present and its associated Cauchy horizon. It is argued that the divergence of the stress-energy scalars for most wave modes makes the nonscalar curvature singularity unstable in general. However, a special subset of modes does not lead to divergence of the stress-energy scalars at the nonscalar singularity. These modes would leave the nonscalar curvature singularity unchanged. Furthermore, examination of the stress-energy tensor in a parallel-propagated orthonormal frame and stress-energy scalars show that the Cauchy horizon is left unchanged.

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