### 抄録

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 |

巻 | 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

### これを引用

**Gravitational waves from a chaotic dynamical system.** / Kiuchi, Kenta; Maeda, Keiichi.

研究成果: Article

*Physical Review D - Particles, Fields, Gravitation and Cosmology*, 巻. 70, 番号 6, 064036. https://doi.org/10.1103/PhysRevD.70.064036

}

TY - JOUR

T1 - Gravitational waves from a chaotic dynamical system

AU - Kiuchi, Kenta

AU - Maeda, Keiichi

PY - 2004

Y1 - 2004

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=84927765649&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84927765649&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.70.064036

DO - 10.1103/PhysRevD.70.064036

M3 - Article

AN - SCOPUS:84927765649

VL - 70

JO - Physical review D: Particles and fields

JF - Physical review D: Particles and fields

SN - 0556-2821

IS - 6

M1 - 064036

ER -