Isospin asymmetry in holographic baryonic matter

We study baryonic matter with isospin asymmetry, including fully dynamically its interplay with pion condensation. To this end, we employ the holographic Witten-Sakai-Sugimoto model and the so-called homogeneous ansatz for the gauge fields in the bulk to describe baryonic matter. Within the confi...

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Main Author: Nicolas Kovensky, Andreas Schmitt
Format: Article
Language:English
Published: SciPost 2021-08-01
Series:SciPost Physics
Online Access:https://scipost.org/SciPostPhys.11.2.029
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author Nicolas Kovensky, Andreas Schmitt
author_facet Nicolas Kovensky, Andreas Schmitt
author_sort Nicolas Kovensky, Andreas Schmitt
collection DOAJ
description We study baryonic matter with isospin asymmetry, including fully dynamically its interplay with pion condensation. To this end, we employ the holographic Witten-Sakai-Sugimoto model and the so-called homogeneous ansatz for the gauge fields in the bulk to describe baryonic matter. Within the confined geometry and restricting ourselves to the chiral limit, we map out the phase structure in the presence of baryon and isospin chemical potentials, showing that for sufficiently large chemical potentials condensed pions and isospin-asymmetric baryonic matter coexist. We also present first results of the same approach in the deconfined geometry and demonstrate that this case, albeit technically more involved, is better suited for comparisons with and predictions for real-world QCD. Our study lays the ground for future improved holographic studies aiming towards a realistic description of charge neutral, beta-equilibrated matter in compact stars, and also for more refined comparisons with lattice studies at nonzero isospin chemical potential.
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spelling doaj.art-045ac96f9b004e5ea7c0918bc29ebf032022-12-21T20:13:33ZengSciPostSciPost Physics2542-46532021-08-0111202910.21468/SciPostPhys.11.2.029Isospin asymmetry in holographic baryonic matterNicolas Kovensky, Andreas SchmittWe study baryonic matter with isospin asymmetry, including fully dynamically its interplay with pion condensation. To this end, we employ the holographic Witten-Sakai-Sugimoto model and the so-called homogeneous ansatz for the gauge fields in the bulk to describe baryonic matter. Within the confined geometry and restricting ourselves to the chiral limit, we map out the phase structure in the presence of baryon and isospin chemical potentials, showing that for sufficiently large chemical potentials condensed pions and isospin-asymmetric baryonic matter coexist. We also present first results of the same approach in the deconfined geometry and demonstrate that this case, albeit technically more involved, is better suited for comparisons with and predictions for real-world QCD. Our study lays the ground for future improved holographic studies aiming towards a realistic description of charge neutral, beta-equilibrated matter in compact stars, and also for more refined comparisons with lattice studies at nonzero isospin chemical potential.https://scipost.org/SciPostPhys.11.2.029
spellingShingle Nicolas Kovensky, Andreas Schmitt
Isospin asymmetry in holographic baryonic matter
SciPost Physics
title Isospin asymmetry in holographic baryonic matter
title_full Isospin asymmetry in holographic baryonic matter
title_fullStr Isospin asymmetry in holographic baryonic matter
title_full_unstemmed Isospin asymmetry in holographic baryonic matter
title_short Isospin asymmetry in holographic baryonic matter
title_sort isospin asymmetry in holographic baryonic matter
url https://scipost.org/SciPostPhys.11.2.029
work_keys_str_mv AT nicolaskovenskyandreasschmitt isospinasymmetryinholographicbaryonicmatter