Regularization of Gravitational Radiation Reaction Force

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概要

• 論文の詳細を見る

• A particle with negligible mass is known to move along a geodesic of a background spacetime. We discuss the leading correction to the equation of motion due to the mass of the particle and its explicit derivation when the background metric is a Schwarzchild/Kerrgeometry. This paper focuses on the metric perturbation only around the particle and proposes a new method to derive a finite radiation reaction force to the particle motion. An advantage of this method is that it is possible to calculate the adiabatic evolution of all kinds of bound orbits. In order to verify this method, we consider the radiation reaction to a particle in a circular orbit around a Schwarzschild black hole.

• 理論物理学刊行会の論文
• 1998-01-25

著者

• Mino Ysushi

  Dpartment Of Earth And Space Science Graduate School Of Science Osaka University

• MINO Ysushi

  Dpartment of Earth and Space Science, Graduate School of Science Osaka University

• Mino Yasushi

  Dpartment of Earth and Space Science, Graduate School of Science Osaka University

関連論文

• Covariant Self-Force Regularization of a Particle Orbiting a Schwarzschild Black Hole : Mode Decomposition Regularization(Astrophysics and Relativity)
• Self-Force on a Scalar Charge in Circular Orbit around a Schwarzschild Black Hole
• Chapter 1 Black Hole Perturbation
• Regularization of Gravitational Radiation Reaction Force
• Chapter 7 Gravitational Radiation Reaction
• Regularization Method of Gravitational Radiation Reaction : Astrophysics and Relativity

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