{
  "id": "2011.11686",
  "version": "v1",
  "published": "2020-11-23T19:24:53.000Z",
  "updated": "2020-11-23T19:24:53.000Z",
  "title": "Deconfinement Phase Transition under Chemical Equilibrium",
  "authors": [
    "Veronica Dexheimer",
    "Krishna Aryal",
    "Madison Wolf",
    "Constantinos Constantinou",
    "Ricardo L. S. Farias"
  ],
  "categories": [
    "nucl-th",
    "astro-ph.HE",
    "astro-ph.SR",
    "hep-th"
  ],
  "abstract": "In this work, we investigate how the assumption of chemical equilibrium with leptons affects the deconfinement phase transition to quark matter. This is done within the framework of the Chiral Mean Field model (CMF) allowing for non-zero net strangeness, corresponding to the conditions found in astrophysical scenarios. We build 3-dimensional QCD phase diagrams with temperature, baryon chemical potential, and either charge or isospin fraction or chemical potential to show how the deconfinement region collapses to a line in the special case of chemical equilibrium, such as the one established the interior of cold catalyzed neutron stars.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-11-23T19:24:53.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "deconfinement phase transition",
      "chemical equilibrium",
      "chiral mean field model",
      "non-zero net strangeness",
      "qcd phase diagrams"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}