Stability criterion for cold stars

Details Stability criterion for cold stars Stability criterion for cold stars

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980afz....16..743b&link_type=abstract

(Astrofizika, vol. 16, Oct.-Dec. 1980, p. 743-749.) Astrophysics, vol. 16, no. 4, Apr. 1981, p. 426-430. Translation.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Dynamic Stability, Relativistic Effects, Stellar Mass Accretion, Baryons, Integral Equations, Mass Distribution

Scientific paper

It is shown that the Zel'dovich-Novikov (1971) stability criterion for cold stars is valid for relativistic configurations. The method for determining this stability is based on the comparison of the internal structure of configurations with similar values of the pressure at the center. Some illustrations of the stability criterion are presented; particular attention is given to solutions corresponding to baryon configurations.

Affiliated with

Also associated with

No associations

Rating

Stability criterion for cold stars 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 Stability criterion for cold stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability criterion for cold stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-947167