Nonlinear evolutions of bosonic clouds around black holes

Hirotada Okawa*

*この研究の対応する著者

研究成果: Article査読

3 被引用数 (Scopus)

抄録

Black holes are a laboratory not only for testing the theory of gravity but also for exploring the properties of fundamental fields. Fundamental fields around a supermassive black hole give rise to extremely long-lived quasi-bound states which can in principle extract the energy and angular momentum from the black hole. To investigate the final state of such a system, the backreaction onto the spacetime becomes important because of the nonlinearity of the Einstein equation. In this paper, we review the numerical method to trace the evolution of massive scalar fields in the vicinity of black holes, how such a system originates from scalar clouds initially in the absence of black holes or from the capture of scalar clouds by a black hole, and the evolution of quasi-bound states around both a non-rotating black hole and a rotating black hole including the backreaction.

本文言語English
論文番号214003
ジャーナルClassical and Quantum Gravity
32
21
DOI
出版ステータスPublished - 2015 10月 15

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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