Rotating shell model of a relativistic star

Details Rotating shell model of a relativistic star Rotating shell model of a relativistic star

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978dossr.243...78l&link_type=abstract

(Akademiia Nauk SSSR, Doklady, vol. 243, Nov. 1, 1978, p. 78-81.) Soviet Physics - Doklady, vol. 23, Nov. 1978, p. 834, 835. Tra

Physics

Mathematical Models, Relativistic Plasmas, Rotating Spheres, Spherical Shells, Stellar Atmospheres, Adiabatic Conditions, Angular Velocity, Hydrodynamic Equations, Particle Density (Concentration), Schwarzschild Metric

Scientific paper

The model proposed for the rotating atmosphere of a relativistic star is
an exact solution of the relativistic hydrodynamic equations of an ideal
fluid situated in a centrally symmetrical statistical gravitational
field. This field is assumed to be generated by a massive central body,
whose radius need not be greater than the Schwarzschild radius.

Affiliated with

Also associated with

No associations

Rating

Rotating shell model of a relativistic star 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 Rotating shell model of a relativistic star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotating shell model of a relativistic star will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1067109