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  On the equation of motion of compact binaries in the post-Newtonian approximation

Itoh, Y. (2004). On the equation of motion of compact binaries in the post-Newtonian approximation. Classical Quantum Gravity, 21(5), S529-S534.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5038-1 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5039-0
Genre: Conference Paper

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118629.pdf (Preprint), 133KB
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 Creators:
Itoh, Yousuke1, 2, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              
2MPI for Gravitational Physics, Max Planck Society, ou_24007              

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 Abstract: A third post-Newtonian (3 PN) equation of motion for two spherical compact stars in a harmonic coordinate has been derived based on the surface integral approach and the strong field point particle limit. The strong field point particle limit enables us to incorporate a notion of a self-gravitating regular star into general relativity. The resulting 3 PN equation of motion is Lorentz invariant, unambiguous, and conserves the energy of the binary orbital motion.

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Language(s): eng - English
 Dates: 2004-03-07
 Publication Status: Published in print
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 Identifiers: eDoc: 118629
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Title: 5th Edoardo Amaldi Conference on Gravitational Waves
Place of Event: Tirrenia, Italy
Start-/End Date: 2003-07-06 - 2003-07-11

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Title: Classical Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 21 (5) Sequence Number: - Start / End Page: S529 - S534 Identifier: -