The Specific Heat of Normal, Degenerate Quark Matter: Non-Fermi Liquid Corrections
arXiv:hep-ph/0011354 · doi:10.1103/PhysRevD.63.114028
Abstract
In normal degenerate quark matter, the exchange of dynamically screened transverse gluons introduces infrared divergences in the quark self-energies that lead to the breakdown of the Fermi liquid description. If the core of neutron stars are composed of quark matter with a normal component, cooling by direct quark Urca processes may be modified by non-Fermi liquid corrections. We find that while the quasiparticle density of states is finite and non-zero at the Fermi surface, its frequency derivative diverges and results in non-Fermi liquid corrections to the specific heat of the normal, degenerate component of quark matter. We study these non-perturbative non-Fermi liquid corrections to the specific heat and the temperature dependence of the chemical potential and show that these lead to a reduction of the specific heat.
new discussion, updated references, accepted in PRD
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- Anomalous specific heat in high-density QED and QCD
- Thermodynamics of Large-N_f QCD at Finite Chemical Potential
- Fermionic dispersion relations in ultradegenerate relativistic plasmas beyond leading logarithmic order
- Non-Fermi liquid corrections to the neutrino mean free path in dense quark matter
- Dynamics near the critical point: the hot renormalization group in quantum field theory
- Spontaneous magnetization in QCD and non-Fermi-liquid effects
- Non-Fermi liquid behavior of the drag and diffusion coefficients in QED plasma
- Non-Fermi-liquid effect in magnetic susceptibility
- Thermodynamics of QCD at large quark chemical potential