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In this work we have derived the expressions of the mean free path (MFP) andemissivity of the neutrinos by incorporating non-Fermi liquid (NFL) correctionsupto next to leading order (NLO). We have shown how such corrections affect thecooling of the neutron star composed of quark matter core.Comment: Published in the Proceedings of the International Conference on  Recent Trends in Nuclear Physics-2012, Indi

Non-Fermi liquid correction to the neutrino mean free path and emissivity in neutron star beyond the leading order