On the oscillations of dissipative superfluid neutron stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

23 pages, 1 eps Figure

Scientific paper

10.1103/PhysRevD.79.103009

We investigate the oscillations of slowly rotating superfluid stars, taking into account the vortex mediated mutual friction force that is expected to be the main damping mechanism in mature neutron star cores. Working to linear order in the rotation of the star, we consider both the fundamental f-modes and the inertial r-modes. In the case of the (polar) f-modes, we work out an analytic approximation of the mode which allows us to write down a closed expression for the mutual friction damping timescale. The analytic result is in good agreement with previous numerical results obtained using an energy integral argument. We extend previous work by considering the full range of permissible values for the vortex drag, e.g. the friction between each individual vortex and the electron fluid. This leads to the first ever results for the f-mode in the strong drag regime. Our estimates provide useful insight into the dependence on, and relevance of, various equation of state parameters. In the case of the (axial) r-modes, we confirm the existence of two classes of modes. However, we demonstrate that only one of these sets remains purely axial in more realistic neutron star models. Our analysis lays the foundation for companion studies of the mutual friction damping of the r-modes at second order in the slow-rotation approximation, the first time evolutions for superfluid neutron star perturbations and also the first detailed attempt at studying the dynamics of superfluid neutron stars with both a relative rotation between the components and mutual friction.

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

On the oscillations of dissipative superfluid 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 On the oscillations of dissipative superfluid neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the oscillations of dissipative superfluid neutron stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-227050

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