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Quantum singularities in self-similar spacetimes

  • D. A. KonkowskiEmail author
  • J. Williams
  • T. M. Helliwell
Research Article
  • 78 Downloads

Abstract

Singularities, which are commonplace in general relativity, are indicated by causal geodesic incompleteness in otherwise maximal spacetimes. Can such singularities be healed (or “resolved”) quantum mechanically? Geodesics are in effect the paths of classical particles, which led Horowitz and Marolf to propose that they be replaced by quantum wave packets. Then a singularity is healed if the quantum wave operator can be shown to be essentially self-adjoint. We explore here a generalized Horowitz–Marolf approach for conformally static spacetimes in the context of the Klein–Gordon operator in the vicinity of singularities in the self-similar spacetimes introduced by Brady. We show that it fails the self-adjointness test for an entire generic class of spacetimes that have asymptotically power-law metric coefficients near the classically-singular origin, so the singularities in these spacetimes cannot be healed using quantum wave packets.

Keywords

Quantum singularities Essential self-adjointness Self-similar spacetimes Scalar curvature singularities 

Notes

Acknowledgements

One of us (DAK) thanks Queen Mary University of London, where some of this research was carried out, for their hospitality.

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Copyright information

© Springer Science+Business Media, LLC, part of Springer Nature 2018

Authors and Affiliations

  1. 1.Department of MathematicsU.S. Naval AcademyAnnapolisUSA
  2. 2.Department of PhysicsHarvey Mudd CollegeClaremontUSA

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