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Phys. Rev. D 76, 024003 (2007) [9 pages]

Numerical simulations of gravitational collapse in Einstein-aether theory

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David Garfinkle*
Department of Physics, Oakland University, Rochester, Michigan 48309, USA

Christopher Eling and Ted Jacobson
Department of Physics, University of Maryland, College Park, Maryland 20742, USA

Received 20 March 2007; published 6 July 2007

We study gravitational collapse of a spherically symmetric scalar field in Einstein-aether theory (general relativity coupled to a dynamical unit timelike vector field). The initial value formulation is developed, and numerical simulations are performed. The collapse produces regular, stationary black holes, as long as the aether coupling constants are not too large. For larger couplings a finite area singularity occurs. These results are shown to be consistent with the stationary solutions found previously.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.76.024003
DOI:
10.1103/PhysRevD.76.024003
PACS:
04.50.+h, 04.25.Dm, 04.70.Bw

*garfinkl@oakland.edu

cteling@physics.umd.edu

jacobson@umd.edu