Gravitational waves from a chaotic dynamical system

Kenta Kiuchi, Keiichi Maeda

    研究成果: Article

    21 引用 (Scopus)

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    To investigate how chaos affects gravitational waves, we study the gravitational waves from a spinning test particle moving around a Kerr black hole, which is a typical chaotic system. To compare the result with those in a nonchaotic dynamical system, we also analyze a spinless test particle, whose orbit can be complicated in the Kerr back ground although the system is integrable. We estimate the emitted gravitational waves by the multipole expansion of a gravitational field. We find a striking difference in the energy spectra of the gravitational waves. The spectrum for a chaotic orbit of a spinning particle contains various frequencies, while some characteristic frequencies appear in the case of a spinless particle.

    元の言語English
    記事番号064036
    ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
    70
    発行部数6
    DOI
    出版物ステータスPublished - 2004

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    ASJC Scopus subject areas

    • Physics and Astronomy(all)
    • Nuclear and High Energy Physics
    • Mathematical Physics

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