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

In this work we have derived the expressions of the mean free path (MFP) and emissivity of the neutrinos by incorporating non-Fermi liquid (NFL) corrections upto next to leading order (NLO). We have shown how such corrections affect the cooling of the neutron star composed of quark matter core.

preprint2013arXivOpen access

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