QCD at finite isospin density: Chiral perturbation theory confronts lattice data

Prabal Adhikari,Jens O Andersen

doi:10.1016/j.physletb.2020.135352

Abstract

We consider the thermodynamics of three-flavor QCD in the pion-condensed phase at nonzero isospin chemical potential (μI) and vanishing temperature using chiral perturbation theory in the isospin limit. The transition from the vacuum phase to a superfluid phase with a Bose-Einstein condensate of charged pions is shown to be second order and takes place at μI=mπ. We calculate the pressure, isospin density, and energy density to next-to-leading order in the low-energy expansion. Our results are compared with recent high-precision lattice simulations as well as previously obtained results in two-flavor chiral perturbation theory. The agreement between the lattice results and the predictions from three-flavor chiral perturbation theory is very good for μI<200 MeV. For larger values of μI, the agreement between lattice data and the two-flavor predictions is surprisingly good and better than with the three-flavor predictions. Finally, in the limit ms≫mu=md, we show that the three-flavor observables reduce to the two-flavor observables with renormalized parameters. The disagreement between the results for two-flavor and three-flavor χPT can largely be explained by the differences in the measured low-energy constants.

Highlights

QCD in extreme conditions, i.e. high temperature and density has received a lot of attention in the past decades due to its relevance to the early universe, heavy-ion collisions, and compact stars [1,2,3]
The expressions for the effective potential, isospin density, pressure, and energy density are all expressed in terms of the isospin chemical potential, the parameters B0m, B0ms, and f of the chiral Lagrangian as well as the renormalized couplings Lri
The results are expressed in terms of

Summary

Introduction

QCD in extreme conditions, i.e. high temperature and density has received a lot of attention in the past decades due to its relevance to the early universe, heavy-ion collisions, and compact stars [1,2,3]. We calculate the effective potential in chiral perturbation theory at next-to-leading (NLO) order in the low-energy expansion for three flavors at finite isospin chemical potential. The last term in Eq (11) is a contact term, which is needed to renormalize the vacuum energy and to show the scale independence of the final result for the effective potential in each phase.

Results

Conclusion