This data reference paper summarizes the fundamental calculated results obtained analytically for the case of a neutron star (NS) crust: it’s cooling rate, time-scale evolution and neutrino luminosity, based on two different theories- Photo-Neutrino (PN) interaction and conventional weak interaction. Considering the NS environment as a degenerate plasmon composition the calculation tables are given.

{"references": ["Majumder, Brajagopal. PhD thesis: Some aspects of stellar neutrino emission in a strong magnetic field from the view point of photo-neutrino weak coupling theory. Awarded by Calcutta University, India."]}