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Cited by 186

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Ergoregion instability of ultracompact astrophysical objects

Open access
Cardoso, Vitor, Pani, Paolo, Cadoni, Mariano, Cavaglià, Marco·2008·Physical Review D

Abstract

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 $M=1\ensuremath{-}{10}^{6}{M}_{\ensuremath{\bigodot}}$ and angular momentum $J>0.4{M}^{2}$. 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.

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Metadata

Authors
Cardoso, V., Pani, P., Cadoni, M., & Cavaglià, M.
Venue
Physical Review D
Published
2008-06-26
Volume
77
Issue
12
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W2154217747
Cited by
186
References
2
FWCI
3.34
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Ergoregion instability of ultracompact astrophysical objects. https://app.cochat.ai/papers/10.1103/physrevd.77.124044
The paper
Cardoso, V., Pani, P., Cadoni, M., & Cavaglià, M. (2008). Ergoregion instability of ultracompact astrophysical objects. Physical Review D. https://doi.org/10.1103/physrevd.77.124044

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.