arXiv:1304.2546·v1·High Energy Physics — Phenomenology
Non-Fermi liquid correction to the neutrino mean free path and emissivity in neutron star beyond the leading order
Souvik Priyam Adhya🇮🇳 · Pradip K. Roy🇮🇳 · Abhee K. Dutt-Mazumder🇮🇳
Abstract
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.
Comments: Published in the Proceedings of the International Conference on Recent Trends in Nuclear Physics-2012, India