Statistics – Computation
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...79..189t&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 79, no. 2, Aug. 1989, p. 189-203. Research supported by the
Statistics
Computation
3
Computational Astrophysics, Condensed Matter Physics, Neutron Stars, Relativistic Effects, Stellar Rotation, Stellar Structure, Binary Stars, Equations Of State, Numerical Integration, Pulsars, Stellar Models
Scientific paper
A broad numerical survey of relativistic rotating neutron star structures was compiled using an exhaustive list of presently available equation of state models for neutron star matter. The structure parameters (spherical deformations in mass and radii, the moment of inertia and quadrupole moment, oblateness, and free precession) are calculated using the formalism proposed by Hartle and Thorne (1968). The results are discussed in relation to the relevant observational information. Binary pulsar data and X-ray burst sources provide information on the bulk properties of neutron stars, enabling the derivation of constraints that can be put on the structure of neutron stars and equation of state models.
No associations
LandOfFree
A numerical survey of relativistic rotating neutron star structures using the Hartle-Thorne formalism 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 A numerical survey of relativistic rotating neutron star structures using the Hartle-Thorne formalism, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A numerical survey of relativistic rotating neutron star structures using the Hartle-Thorne formalism will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1514037