Post-Newtonian expansion of gravitational waves from a particle in circular orbit around a rotating black hole: Up to<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>O</mml:mi><mml:mo>(</mml:mo><mml:mrow><mml:msup><mml:mrow><mml:mi>v</mml:mi></mml:mrow><mml:mrow><mml:mn>8</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mo>)</mml:mo></mml:math>beyond the quadrupole formula
Hideyuki Tagoshi(Osaka Health Science University), Misao Sasaki(Kavli Institute for the Physics and Mathematics of the Universe), Masaru Shibata(Instituto de Física Teórica), Takahiro Tanaka(The University of Osaka)
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
July 15, 1996
Cited by 74
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