Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Display Documents



  history
ID: 118629.0, MPI für Gravitationsphysik / Astrophysical Relativity
On the equation of motion of compact binaries in the post-Newtonian approximation
Authors:Itoh, Yousuke
Language:English
Date of Publication (YYYY-MM-DD):2004-03-07
Title of Journal:Classical Quantum Gravity
Volume (in Journal):21
Issue / Number:5
Start Page:S529
End Page:S534
Name of Conference/Meeting:5th Edoardo Amaldi Conference on Gravitational Waves
Place of Conference/Meeting:Tirrenia, Italy
(Start) Date of Conference/Meeting
 (YYYY-MM-DD):
2003-07-06
End Date of Conference/Meeting 
 (YYYY-MM-DD):
2003-07-11
Review Status:not specified
Audience:Not Specified
Abstract / Description: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.
External Publication Status:published
Document Type:Conference-Paper
Communicated by:Bernhard F. Schutz
Affiliations:MPI für Gravitationsphysik/Astrophysical Relativity
MPI für Gravitationsphysik
Full Text:
You have privileges to view the following file(s):
118629.pdf  [132,00 Kb] [Comment:arXiv]  
 
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.