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Phys. Rev. D 77, 124044 (2008) [15 pages]

Ergoregion instability of ultracompact astrophysical objects

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Vitor Cardoso*
Department of Physics and Astronomy, The University of Mississippi, University, Mississippi 38677-1848, USA

Paolo Pani
Dipartimento di Fisica, Università di Cagliari, Cittadella Universitaria 09042 Monserrato, Italy, and Department of Physics and Astronomy, The University of Mississippi, University, Mississippi 38677-1848, USA

Mariano Cadoni
Dipartimento di Fisica, Università di Cagliari, and INFN sezione di Cagliari, Cittadella Universitaria 09042 Monserrato, Italy

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

Received 15 September 2007; published 26 June 2008

Most of the properties of black holes can be mimicked by horizonless compact objects such as gravastars and boson stars. We show that these ultracompact objects develop a strong ergoregion instability when rapidly spinning. Instability time scales can be of the order of 0.1 seconds to 1 week for objects with mass M=1-106M and angular momentum J>0.4M2. This provides a strong indication that ultracompact objects with large rotation are black holes. Explosive events due to ergoregion instability have a well-defined gravitational-wave signature. These events could be detected by next-generation gravitational-wave detectors such as Advanced LIGO or LISA.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.77.124044
DOI:
10.1103/PhysRevD.77.124044
PACS:
04.40.Dg, 04.25.Nx, 04.30.Nk, 95.85.Sz

*Presently at CENTRA, Department de Física, Instituto Superior Técnico, Avenida Rovisco Pais 1, 1049-001 Lisboa, Portugal.

vcardoso@phy.olemiss.edu

paolo.pani@ca.infn.it

mariano.cadoni@ca.infn.it

§cavaglia@phy.olemiss.edu