High precision rotating neutron star models. II. Large sample of neutron star properties.

Details High precision rotating neutron star models. II. Large sample of neutron star properties. High precision rotating neutron star models. II. Large sample of neutron star properties.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..108..455s&link_type=abstract

Astronomy and Astrophysics Suppl. 108, 455-459 (1994)

Astronomy and Astrophysics

Astrophysics

38

Relativity, Stars: Neutron, Rotation, Pulsars, Equations Of State

Scientific paper

A new and highly precise numerical approach for computing stationary rotating stellar configurations in general relativity has been employed to construct rotating neutron star models. Fourteen equations of state (EOS) of cold dense matter have been used to produce a "catalog" of thousands neutron star models, parametrized by the EOS, the central energy density and the angular velocity. The results are presented in a series of tables for each EOS. A particular emphasis is put on the properties of maximal mass models. These latter are useful to constrain the EOS, taking into account the observed pulsars.

Affiliated with

Also associated with

No associations

Rating

High precision rotating neutron star models. II. Large sample of neutron star properties. 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 High precision rotating neutron star models. II. Large sample of neutron star properties., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High precision rotating neutron star models. II. Large sample of neutron star properties. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1318159