Non-Fermi liquid corrections to the neutrino mean free path in dense quark matter

Abstract

We calculate the neutrino mean free path with non-Fermi liquid (NFL) corrections in quark matter from scattering and absorption processes for both degenerate and nondegenerate neutrinos. We show that the mean free path decreases due to the non-Fermi liquid corrections leading to $l_{mean}^{-1}\sim [......+....C_F^2{\alpha }_s^2\ln (m_D/T{)}^2]$. These reduction results in higher rate of scattering.

12 pages, 2 eps figures, published in PRD

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Cited by in corpus (9)

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• Next to leading order non Fermi liquid corrections to the neutrino emissivity and cooling of the neutron star
• Modifications to the pulsar kick velocity due to magnetic interactions in dense plasma
• When cold, dense quarks in 1+1 and 3+1 dimensions are not a Fermi liquid
• Non-Fermi liquid behavior of the drag and diffusion coefficients in QED plasma
• Neutrino beaming in ultraluminous X-ray pulsars as a result of gravitational lensing by neutron stars
• Non-Fermi liquid behavior of thermal relaxation time in degenerate electron plasma
• Neutrino diffusive transport in hot quark matter: a detailed analysis
• Astrophysical aspects of neutrino dynamics in ultra-degenerate quark gluon plasma