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A general relativistic Thomas-Fermi treatment of neutron star cores
Proceedings of 25th Texas Symposium on Relativistic Astrophysics — PoS(Texas 2010)
We formulate the set of self-consistent ground-state equilibrium equations for neutron star cores taking into account quantum statistics, electro-weak, and strong interactions, within the framework of general relativity. The strong interaction between nucleons is modeled through the sigmaomega-rho meson exchange in the context of the extended Walecka model, all duly expressed in general relativity. We found the generalization to the works of Klein (1949), of Kodama and Yamada (1972) , and ofdoi:10.22323/1.123.0271 fatcat:ywbnzm3xxrhbtl64o3h6sm2zki