Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations

Details Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..35.2287s&link_type=abstract

Physical Review D (Particles and Fields), Volume 35, Issue 8, 15 April 1987, pp.2287-2296

Physics

34

Scientific paper

Odd-parity gravitational perturbations of a spherically symmetric background are studied in the linearized Einstein theory. A variety of collapse models, based on a May-White hydrodynamic code, are investigated, simulating dust collapse and stellar core collapse typical of type-II supernova models. Numerical results are presented, showing that in this linearized problem a typical core collapse may radiate up to 10-7 Mc2 in gravitational-wave energy.

Affiliated with

Also associated with

No associations

Rating

Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations 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 from realistic relativistic stars: Odd-parity fluid perturbations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1349775