Thermodynamics of two-flavor isospin-asymmetric superfluid quark matter at next-to-leading order
Abstract
We study quark matter at high isospin asymmetry in the limit of vanishing baryon density, a state of matter governed by the condensation of charged pions. In the weak-coupling limit, this state of matter can be reliably described by conventional perturbative methods where a trivial ground state is assumed. However, since the condensate of charged pions generates a gap in the excitation spectrum of the quarks with a non-perturbative dependence on the strong coupling, corrections to the results from conventional perturbative methods arise. This situation is very reminiscent of the one encountered in isospin-symmetric quark matter at high baryon densities which is expected to be a color superconductor. In the present work, we calculate the thermodynamic properties of superfluid quark matter at high isospin asymmetry, zero temperature, and zero baryon density at next-to-leading order (NLO) in the coupling in the presence of a finite gap. We work in the limit of two massless quark flavors and further assume that the gap is small compared to the isospin chemical potential. Similar to the situation in color-superconducting quark matter at high baryon densities, we find that the gap-induced corrections lead to an increase of the pressure and the speed of sound above their values obtained for non-superfluid quark matter. Notably, starting from asymptotically high isospin asymmetries, these corrections lead to a systematic change of the slope of the speed of sound when the isospin asymmetry is decreased. We compare our results with recent lattice QCD and Dyson-Schwinger equation studies and find good agreement in the regimes where these methods are applicable.
Related
- Glashow-Weinberg relation in isospin-asymmetric nuclear matter
- Isospin and flavor SU(3) symmetry breaking in doubly heavy baryons
- Testing strong isospin breaking effects in QCD thermodynamics
- Diffusion and shear viscosity coefficients of hot isospin asymmetric strange hadronic matter using a chiral SU(3) model
- Parton distribution functions of the proton in a hot isospin-asymmetric nuclear medium and finite nuclei
BibTeX
@misc{rehbergjuditzky2026thermodynamics,
title = {{Thermodynamics of two-flavor isospin-asymmetric superfluid quark matter at next-to-leading order}},
author = {Tim Rehberg-Juditzky and Andreas Geißel and Jens Braun},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.25882},
eprint = {2610.25882},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.25882},
}
RIS
TY - UNPB
TI - Thermodynamics of two-flavor isospin-asymmetric superfluid quark matter at next-to-leading order
AU - Tim Rehberg-Juditzky
AU - Andreas Geißel
AU - Jens Braun
PY - 2026
DA - 2026/10/19
PB - arXiv
DO - 10.48550/arxiv.2610.25882
UR - https://arxiv.org/abs/2610.25882
AB - We study quark matter at high isospin asymmetry in the limit of vanishing baryon density, a state of matter governed by the condensation of charged pions. In the weak-coupling limit, this state of matter can be reliably described by conventional perturbative methods where a trivial ground state is assumed. However, since the condensate of charged pions generates a gap in the excitation spectrum of the quarks with a non-perturbative dependence on the strong coupling, corrections to the results from conventional perturbative methods arise. This situation is very reminiscent of the one encountered in isospin-symmetric quark matter at high baryon densities which is expected to be a color superconductor. In the present work, we calculate the thermodynamic properties of superfluid quark matter at high isospin asymmetry, zero temperature, and zero baryon density at next-to-leading order (NLO) in the coupling in the presence of a finite gap. We work in the limit of two massless quark flavors and further assume that the gap is small compared to the isospin chemical potential. Similar to the situation in color-superconducting quark matter at high baryon densities, we find that the gap-induced corrections lead to an increase of the pressure and the speed of sound above their values obtained for non-superfluid quark matter. Notably, starting from asymptotically high isospin asymmetries, these corrections lead to a systematic change of the slope of the speed of sound when the isospin asymmetry is decreased. We compare our results with recent lattice QCD and Dyson-Schwinger equation studies and find good agreement in the regimes where these methods are applicable.
ER -