Other
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197..845i&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 197, Dec. 1981, p. 845-864.
Other
3
Neutron Stars, Stellar Mass Ejection, Stellar Structure, Stellar Temperature, Degenerate Matter, Equations Of State, Gibbs Free Energy, Isothermal Processes, Moments Of Inertia, Red Shift, Stellar Gravitation
Scientific paper
Using Lamb's (1969) equations of state for warm neutron degenerate matter, relativistic equations of structure are solved. The stability of isothermal cores in neutron stars is discussed, and the possible compatibility of the results obtained with experimental evidence is shown. Here, the leptonic pressure is derived from the standard Fermi-Dirac statistics, and the chemical potential of nucleons is obtained by following the perturbation approach employed by Langer et al. (1969, 1970) and then by splitting each nucleon Gibbs energy into a free-particle Gibbs energy and and interaction energy. The nucleon-nucleon interaction is described through the velocity-dependent potential of Weiss and Cameron (1969).
No associations
LandOfFree
Structure and stability of warm cores in 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 Structure and stability of warm cores in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure and stability of warm cores in neutron stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1264665