Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-09-20
Phys.Rev. D65 (2002) 084039
Astronomy and Astrophysics
Astrophysics
RevTeX 4, 17 pages, 26 figures. Slightly revised. To be published in PRD (April 2002)
Scientific paper
10.1103/PhysRevD.65.084039
Nonlinear evolution of the gravitational radiation (GR) driven instability in the r-modes of neutron stars is studied by full numerical 3D hydrodynamical simulations. The growth of the r-mode instability is found to be limited by the formation of shocks and breaking waves when the dimensionless amplitude of the mode grows to about three in value. This maximum mode amplitude is shown by numerical tests to be rather insensitive to the strength of the GR driving force. Upper limits on the strengths of possible nonlinear mode--mode coupling are inferred. Previously unpublished details of the numerical techniques used are presented, and the results of numerous calibration runs are discussed.
Lindblom Lee
Tohline Joel E.
Vallisneri Michele
No associations
LandOfFree
Numerical evolutions of nonlinear r-modes in neutron stars 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 Numerical evolutions of nonlinear r-modes in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical evolutions of nonlinear r-modes in neutron stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-722768