### Abstract

Recently we developed a time-domain code to calculate the gravitational self-force on a point particle moving around a Schwarzschild black hole. To know how the force affects the particle's motion, it is useful to estimate the self-force correction of some characteristic variables of the orbits (e.g. ISCO frequency, periastron shift). In this work, we focus on the self-force effect on the periastron shift and investigate how to evaluate the correction from the numerical results of the self-force with our time-domain code.

Original language | English |
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Pages | 291-294 |

Number of pages | 4 |

Publication status | Published - Dec 1 2009 |

Event | 19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009 - Tokyo, Japan Duration: Nov 30 2009 → Dec 4 2009 |

### Other

Other | 19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009 |
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Country | Japan |

City | Tokyo |

Period | 11/30/09 → 12/4/09 |

### Fingerprint

### All Science Journal Classification (ASJC) codes

- Atomic and Molecular Physics, and Optics

### Cite this

*Gravitational self-force effect on the periastron shift in schwarzschild spacetime*. 291-294. Paper presented at 19th Workshop on General Relativity and Gravitation in Japan, JGRG 2009, Tokyo, Japan.

**Gravitational self-force effect on the periastron shift in schwarzschild spacetime.** / Sago, Norichika; Barack, Leor.

Research output: Contribution to conference › Paper

}

TY - CONF

T1 - Gravitational self-force effect on the periastron shift in schwarzschild spacetime

AU - Sago, Norichika

AU - Barack, Leor

PY - 2009/12/1

Y1 - 2009/12/1

N2 - Recently we developed a time-domain code to calculate the gravitational self-force on a point particle moving around a Schwarzschild black hole. To know how the force affects the particle's motion, it is useful to estimate the self-force correction of some characteristic variables of the orbits (e.g. ISCO frequency, periastron shift). In this work, we focus on the self-force effect on the periastron shift and investigate how to evaluate the correction from the numerical results of the self-force with our time-domain code.

AB - Recently we developed a time-domain code to calculate the gravitational self-force on a point particle moving around a Schwarzschild black hole. To know how the force affects the particle's motion, it is useful to estimate the self-force correction of some characteristic variables of the orbits (e.g. ISCO frequency, periastron shift). In this work, we focus on the self-force effect on the periastron shift and investigate how to evaluate the correction from the numerical results of the self-force with our time-domain code.

UR - http://www.scopus.com/inward/record.url?scp=84887472815&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84887472815&partnerID=8YFLogxK

M3 - Paper

AN - SCOPUS:84887472815

SP - 291

EP - 294

ER -