Kinematics of discretely self-similar spherically symmetric spacetimes

Carsten Gundlach and José M. Martín-García
Phys. Rev. D 68, 064019 – Published 29 September 2003
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Abstract

We summarize the consequences of the twin assumptions of (discrete) self-similarity and spherical symmetry for the global structure of a spacetime. All such spacetimes can be constructed from two building blocks: the “fan” and “splash.” Each building block contains one radial null geodesic that is invariant under the self-similarity (self-similarity horizon).

  • Received 2 June 2003

DOI:https://doi.org/10.1103/PhysRevD.68.064019

©2003 American Physical Society

Authors & Affiliations

Carsten Gundlach*

  • Faculty of Mathematical Studies, University of Southampton, Southampton SO17 1BJ, United Kingdom

José M. Martín-García

  • Faculty of Mathematical Studies, University of Southampton, Southampton SO17 1BJ, United Kingdom
  • Departamento Matemática Aplicada y Métodos Informáticos, ETSI Minas, UPM, Madrid 28003, Spain

  • *Email address: C.Gundlach@maths.soton.ac.uk
  • Email address: J.M.Martin-Garcia@maths.soton.ac.uk

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Vol. 68, Iss. 6 — 15 September 2003

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