Newtonian and post-Newtonian binary neutron star mergers

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3 pages, LaTeX, 2 figures, Proceedings of the 8th Marcel Grossmann Meeting, Jerusalem, June 1997 (World Scientific); mprocl.st

Scientific paper

We present two of our efforts directed toward the numerical analysis of neutron star mergers, which are the most plausible sources for gravitational wave detectors that should begin operating in the near future. First we present Newtonian 3D simulations including radiation reaction (2.5PN) effects. We discuss the gravitational wave signals and luminosity from the merger with/without radiation reaction effects. Second we present the matching problem between post-Newtonian formulations and general relativity in numerical treatments. We prepare a spherical, static neutron star in a post-Newtonian matched spacetime, and find that discontinuities at the matching surface become smoothed out during fully relativistic evolution if we use a proper slicing condition.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Newtonian and post-Newtonian binary neutron star mergers 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 Newtonian and post-Newtonian binary neutron star mergers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Newtonian and post-Newtonian binary neutron star mergers will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-166548

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.