English

Chiral density wave versus pion condensation at finite density

High Energy Physics - Phenomenology 2018-04-18 v2

Abstract

The quark-meson model is often used as an effective low-energy model for QCD to study the chiral transition at finite temperature TT, baryon chemical potential μB\mu_B, and isospin chemical potential μI\mu_I. The parameters of the model are determined by matching the meson and quark masses, as well as the pion decay constant to their physical values using the on-shell and modified minimal subtraction schemes. In this paper, we study the possibility of different phases at zero temperature. In particular, we investigate the competition between an inhomogeneous chiral condensate and a pion condensate. For the inhomogeneity, we use a chiral-density wave ansatz. For a sigma mass of 600600 MeV, we find that an inhomogeneous chiral condensate exist only for pion masses below approximately 37 MeV. We also show that due to our parameter fixing, the onset of pion condensation takes place exactly at μI=12mπ\mu_I={1\over2}m_{\pi} in accordance with exact results.

Keywords

Cite

@article{arxiv.1802.01832,
  title  = {Chiral density wave versus pion condensation at finite density},
  author = {Jens O. Andersen and Patrick Kneschke},
  journal= {arXiv preprint arXiv:1802.01832},
  year   = {2018}
}

Comments

14 pages and 11 figs. v2: Minor changes, matches published version in PRD