A higher stability limit for neutron stars

Details A higher stability limit for neutron stars A higher stability limit for neutron stars

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...205..261b&link_type=abstract

Astrophysical Journal, vol. 205, Apr. 1, 1976, pt. 1, p. 261-267.

Astronomy and Astrophysics

Astronomy

13

Dynamic Stability, Equations Of State, Hyperons, Neutron Stars, Relativistic Theory, Stellar Mass, Stellar Models, Black Holes (Astronomy), Moments Of Inertia, Stellar Rotation, Stellar Structure

Scientific paper

A fully relativistic equation of state for hyperons based on strong interactions fitted to nuclear matter has been used to construct neutron stars. The model yields a maximum stable mass of 2.39 solar masses and a maximum moment of inertia of 3.13 times ten to the forty-fifth g sq cm. The significance of these results and their relation to observations are discussed. The sensitivity of the results, particularly the upper mass limit, due to variations of the input parameters is considered.

Affiliated with

Also associated with

No associations

Rating

A higher stability limit for neutron 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 A higher stability limit for neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A higher stability limit for neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1612100