Many-particle theory of nuclear systems with application to neutron star matter

Physics – Condensed Matter – Statistical Mechanics

Scientific paper

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Many Body Problem, Neutron Scattering, Neutron Stars, Flux Density, Numerical Analysis, Parameterization, Statistical Mechanics, Superconductors, Superfluidity

Scientific paper

The energy-density relation was calculated for pure neutron matter in the density range relevant for neutron stars, using four different hard-core potentials. Calculations are also presented of the properties of the superfluid state of the neutron component, along with the superconducting state of the proton component and the effects of polarization in neutron star matter.

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