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Phys. Rev. D 70, 044010 (2004) [5 pages]

Approximately self-similar critical collapse in 2+1 dimensions

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Marco Cavaglià*
Department of Physics and Astronomy, University of Mississippi, University, Mississippi 38677-1848, USA

Gérard Clément
Laboratoire de Physique Théorique, LAPTH (CNRS), B.P. 110, F-74941, Annecy-le-Vieux Cedex, France

Alessandro Fabbri
Dipartimento di Fisica dell’Università di Bologna and INFN sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy
GReCO, Institut d’Astrophysique de Paris (CNRS), 98bis Boul. Arago, 75014 Paris, France

Received 13 April 2004; published 10 August 2004

Critical collapse of a self-gravitating scalar field in a (2+1)-dimensional spacetime with negative cosmological constant seems to be dominated by a continuously self-similar solution of the field equations without cosmological constant. However, previous studies of linear perturbations in this background were inconclusive. We extend the continuously self-similar solutions to solutions of the field equations with negative cosmological constant, and analyze their linear perturbations. The extended solutions are characterized by a continuous parameter. A suitable choice of this parameter seems to improve the agreement with the numerical results. We also study the dynamics of the apparent horizon in the extended background.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.70.044010
DOI:
10.1103/PhysRevD.70.044010
PACS:
04.20.-q, 04.25.-g, 04.40.-b

*Email address: cavaglia@phy.olemiss.edu

Email address: gclement@lapp.in2p3.fr

Email address: fabbria@bo.infn.it