Scalar Field Probes of Power-Law Space-Time Singularities

Abstract

We analyse the effective potential of the scalar wave equation near generic space-time singularities of power-law type (Szekeres-Iyer metrics) and show that the effective potential exhibits a universal and scale invariant leading x^{-2} inverse square behaviour in the ``tortoise coordinate'' x provided that the metrics satisfy the strict Dominant Energy Condition (DEC). This result parallels that obtained in hep-th/0403252 for probes consisting of families of massless particles (null geodesic deviation, a.k.a. the Penrose Limit). The detailed properties of the scalar wave operator depend sensitively on the numerical coefficient of the x^{-2}-term, and as one application we show that timelike singularities satisfying the DEC are quantum mechanically singular in the sense of the Horowitz-Marolf (essential self-adjointness) criterion. We also comment on some related issues like the near-singularity behaviour of the scalar fields permitted by the Friedrichs extension.

arXiv commentv2: 21 pages, JHEP3.cls, one reference added

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• The Initial State of a Primordial Anisotropic Stage of Inflation
• Penrose Limits vs String Expansions
• Quantum probes of timelike naked singularities in $2+1-$ dimensional power - law spacetimes
• Classical and quantum properties of a 2-sphere singularity
• Stability analysis of (a class of) anisotropic spacetimes
• A New Example of the Effects of a Singular Background on the Zeta Function