Gravitational radiation of stellar configurations consisting of incompressible fluid

Details Gravitational radiation of stellar configurations consisting of incompressible fluid Gravitational radiation of stellar configurations consisting of incompressible fluid

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap.....49..211s&link_type=abstract

Astrophysics, Volume 49, Issue 2, pp.211-217

Astronomy and Astrophysics

Astrophysics

Stars, Neutron-Gravitational Radiation, Stellar Configurations

Scientific paper

This article discusses the gravitational radiation of rotating and oscillating stellar configurations with an incompressible fluid equation of state. The method used here makes it possible to determine the frequencies and amplitudes of the gravitational waves for arbitrary values of the central densities. At the densities corresponding to neutron stars, the major parameters of the gravitational radiation are consistent with previous results from more realistic models. Depending on the central density, stellar configurations with an incompressible fluid can emit gravitational waves over a wide range of frequencies, from 10-2 to 104 Hz.

Affiliated with

Also associated with

No associations

Rating

Gravitational radiation of stellar configurations consisting of incompressible fluid 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 Gravitational radiation of stellar configurations consisting of incompressible fluid, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational radiation of stellar configurations consisting of incompressible fluid will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1158183