Statistics – Computation
Scientific paper
Jan 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242..289b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 15, 1990, p. 289-305.
Statistics
Computation
120
Computational Astrophysics, Gravitational Waves, Relativistic Effects, Computerized Simulation, Einstein Equations, Gravitational Collapse, Gravitational Effects, Hydrodynamics
Scientific paper
An approximate formalism is presented for the equations of evolution of a moderately relativistic self-gravitating fluid which takes into account the dominant (quantitative and qualitative) new effects entailed by Einstein's theory. This (first plus second-and-a-half) post-Newtonian scheme is equivalent to known results of the literature, but casts them in an explicitly 'quasi-Newtonian' form, so that it becomes as easy to implement on a computer as a Newtonian-gravity code for nonrelativistic hydrodynamics. This scheme is completed by a corresponding accurate post-Newtonian gravitational waveform extraction formalism which goes beyond the 'standard quadrupole equation' in including the first relativistic corrections to the emission of gravitational radiation in a form which can be easily implemented numerically. The most important quantitative and qualitative characteristics of the three-dimensional gravitational dynamics and wave generation of a wide range of semirelativistic sources can be studied with minimal computer investment.
Blanchet Luc
Damour Thibault
Schaefer Gerhard
No associations
LandOfFree
Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Post-Newtonian hydrodynamics and post-Newtonian gravitational wave generation for numerical relativity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1563743