Black holes and fundamental fields in numerical relativity

Initial data construction and evolution of bound states

Hirotada Okawa, Helvi Witek, Vitor Cardoso

Research output: Contribution to journalArticle

54 Citations (Scopus)

Abstract

Fundamental fields are a natural outcome in cosmology and particle physics and might therefore serve as a proxy for more complex interactions. The equivalence principle implies that all forms of matter gravitate, and one therefore expects relevant, universal imprints of new physics in strong field gravity, such as that encountered close to black holes. Fundamental fields in the vicinities of supermassive black holes give rise to extremely long-lived, or even unstable, configurations, which slowly extract angular momentum from the black hole or simply evolve nonlinearly over long time scales, with important implications for particle physics and gravitational-wave physics. Here, we perform a fully nonlinear study of scalar-field condensates around rotating black holes. We provide novel ways to specify initial data for the Einstein - Klein - Gordon system, with potential applications in a variety of scenarios. Our numerical results confirm the existence of long-lived bar modes, which act as lighthouses for gravitational wave emission: the scalar field condenses outside the black hole geometry and acts as a constant frequency gravitational-wave source for very long time scales. This effect could turn out to be a potential signature of beyond standard model physics and also a promising source of gravitational waves for future gravitational-wave detectors.

Original languageEnglish
Article number104032
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume89
Issue number10
DOIs
Publication statusPublished - 2014 May 21
Externally publishedYes

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gravitational waves
relativity
physics
scalars
cosmology
condensates
equivalence
angular momentum
signatures
gravitation
detectors
configurations
interactions

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

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