Erratum: The Gravitational Radiation Emitted by a System Consisting of a Point Particle in Close Orbit around a Schwarzschild Black Hole

• 作者: Amos S. Kubeka
• 来源期刊: 现代物理(英文)
• 学科: 地球科学
• 关键词: Black Hole PARTICLE GRAVITATIONAL Radiation NULL INFINITY
• 年，卷（期）: 2013,（8）
• 页码范围: 1119-1122
• 页数: 4页
• 分类号: P1

摘要

We correct from the previous paper: the first, second and third order derivatives of the Bondi metric function J at the ISCO of the binary system consisting of a Schwarzschild black hole and a point particle. Previously, these derivatives where not correctly determined and that resulted in the incorrect determination of the emitted gravitational radiation at null infinity. The now correctly calculated gravitational radiation is now in full agreement with that obtained by the standard 5.5 PN formalism to about ninety eight percent. The small percentage difference observed is due to the slow convergence property of the PN formalism as compared to the null cone formalism, otherwise the results are basically the same.