Gravitational instability of exotic compact objects

Andrea Addazi, Antonino Marcianò, Nicolás Yunes

Research output: Contribution to journalLetter

Abstract

Exotic compact objects with physical surfaces a Planckian distance away from where the horizon would have been are inspired by quantum gravity. Most of these objects are defined by a classical spacetime metric, such as boson stars, gravastars and wormholes. We show that these classical objects are gravitationally unstable because accretion by ordinary and dark matter, and by gravitational waves, forces them to collapse into a black hole by the Hoop conjecture. To avoid collapse, either their surface must be a macroscopic distance away from the horizon, or they must violate the null energy condition.

Original languageEnglish (US)
Article number36
JournalEuropean Physical Journal C
Volume80
Issue number1
DOIs
StatePublished - Jan 1 2020
Externally publishedYes

ASJC Scopus subject areas

  • Engineering (miscellaneous)
  • Physics and Astronomy (miscellaneous)

Fingerprint Dive into the research topics of 'Gravitational instability of exotic compact objects'. Together they form a unique fingerprint.

  • Cite this