Modelling of rotating neutron stars using exact solutions of Einstein's equations

Details Modelling of rotating neutron stars using exact solutions of Einstein's equations Modelling of rotating neutron stars using exact solutions of Einstein's equations

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981acaau...8..831p&link_type=abstract

Acta Astronautica, vol. 8, Aug. 1981, p. 831-838.

Astronomy and Astrophysics

Astronomy

Einstein Equations, Neutron Stars, Relativity, Stellar Models, Stellar Rotation, Baryons, Conservation Laws, Electromagnetic Pulses, Pulsars

Scientific paper

A method is proposed for the construction of new, exact solutions of general relativity equations, and the modeling by means of the solutions of rotating neutron stars. The method is based on the theorem obtained by Pisarenko (1977), according to which Einstein's field equations, together with the baryon number conservation law, have in some connecting region a partial family of exact solutions with arbitrary functions that have real values for a metric with a rotation of general form. Four solutions for modeling rotating neutron stars are constructed.

Affiliated with

Also associated with

No associations

Rating

Modelling of rotating neutron stars using exact solutions of Einstein's equations 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 Modelling of rotating neutron stars using exact solutions of Einstein's equations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modelling of rotating neutron stars using exact solutions of Einstein's equations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1743903