Nucleon Fermi Wavenumber Dependence of The Neutron Star Density on The Cooling Process

Details Nucleon Fermi Wavenumber Dependence of The Neutron Star Density on The Cooling Process Nucleon Fermi Wavenumber Dependence of The Neutron Star Density on The Cooling Process

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1325..217i&link_type=abstract

THE 4TH ASIAN PHYSICS SYMPOSIUM-AN INTERNATIONAL SYMPOSIUM. AIP Conference Proceedings, Volume 1325, pp. 217-220 (2010).

Physics

Neutron Stars, Supernovae, Magnetic Field Effects, Superfluidity, Neutron Stars, Supernovae, Electric And Magnetic Fields, Hydrodynamic Aspects Of Superfluidity, Quantum Fluids

Scientific paper

The correlation between a nucleon Fermi wavenumber and the neutron star density has been studied. By paying attention to the density and the nucleon Fermi wavenumber (especially to their dependence on the critical temperature) we show that it leads to a non-linear equation. The equation is solved then by a modified Newton-Raphson method. The two obtained profiles of critical temperature are of different kinds but of the same tendence. The data extract and the equation is compared and interpreted.

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