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Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University

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Article

Completeness of general pp-wave spacetimes and their impulsive limit

Sämann, C., Steinbauer, R., Švarc, R.

Class. Quantum Grav. 33, 215006 (2016)

doi ↗

Abstract

We investigate geodesic completeness in the full family of pp-wave (or
Brinkmann) spacetimes in their extended and impulsive forms. This class of
geometries contains the recently studied gyratonic pp-waves, modelling the
exterior field of a spinning beam of null particles, as well as N-fronted waves
with parallel rays, which generalize classical pp-waves by allowing for a
general wave surface. The problem of geodesic completeness reduces to the
question of completeness of trajectories on a Riemannian manifold under an
external force field. Building upon respective recent results, we derive completeness
criteria in terms of the spatial asymptotics of the profile function in
the extended case. In the impulsive case, we use a fixed-point argument to
show that, irrespective of the behaviour of the profile function, all geometries
in the class are complete.

Institute authors

Supported by

  • GACR 203/12/0118 — Spacetimes and Fields in Higher Dimensional and Classical Gravity
  • UNCE 204020/2012 — Výzkum Země a vesmíru metodami teoretické, počítačové a experimentální fyziky

BibTeX

@article{UTF596,
  author        = {Sämann, C., Steinbauer, R., Švarc, R.},
  title         = {{Completeness of general pp-wave spacetimes and their impulsive limit}},
  journal       = {Class. Quantum Grav.},
  volume        = {33},
  pages         = {215006},
  year          = {2016},
  doi           = {10.1088/0264-9381/33/21/215006},
}