Hamiltonian formulation of the conservative self-force dynamics in the Kerr geometry

Ryuichi Fujita, Soichiro Isoyama, Alexandre Le Tiec, Hiroyuki Nakano, Norichika Sago, Takahiro Tanaka

研究成果: Contribution to journalArticle査読

16 被引用数 (Scopus)

抄録

We formulate a Hamiltonian description of the orbital motion of a point particle in Kerr spacetime for generic (eccentric, inclined) orbits, which accounts for the effects of the conservative part of the gravitational self-force. This formulation relies on a description of the particle's motion as geodesic in a certain smooth effective spacetime, in terms of (generalized) action-angle variables. Clarifying the role played by the gauge freedom in the Hamiltonian dynamics, we extract the gauge-invariant information contained in the conservative self-force. We also propose a possible gauge choice for which the orbital dynamics can be described by an effective Hamiltonian, written solely in terms of the action variables. As an application of our Hamiltonian formulation in this gauge, we derive the conservative self-force correction to the orbital frequencies of Kerr innermost stable spherical (inclined or circular) orbits. This gauge choice also allows us to establish a 'first law of mechanics' for black-hole-particle binary systems, at leading order beyond the test-mass approximation.

本文言語英語
論文番号134001
ジャーナルClassical and Quantum Gravity
34
13
DOI
出版ステータス出版済み - 6 7 2017

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)

フィンガープリント 「Hamiltonian formulation of the conservative self-force dynamics in the Kerr geometry」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル