Isospin asymmetry in holographic baryonic matter

Autores
Kovensky, Nicolas; Schmitt, Andreas
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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.
Fil: Kovensky, Nicolas. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Schmitt, Andreas. University of Southampton; Reino Unido
Materia
Holographic QCD
QCD Phase Diagram
Isospin Asymmetry
Pion Condensation
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/255861

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spelling Isospin asymmetry in holographic baryonic matterKovensky, NicolasSchmitt, AndreasHolographic QCDQCD Phase DiagramIsospin AsymmetryPion Condensationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We 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.Fil: Kovensky, Nicolas. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Schmitt, Andreas. University of Southampton; Reino UnidoSciPost Foundation2021-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/255861Kovensky, Nicolas; Schmitt, Andreas; Isospin asymmetry in holographic baryonic matter; SciPost Foundation; SciPost Physics; 11; 2; 7-2021; 029, 1-492542-4653CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://scipost.org/SciPostPhys.11.2.029info:eu-repo/semantics/altIdentifier/doi/10.21468/SciPostPhys.11.2.029info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:35:56Zoai:ri.conicet.gov.ar:11336/255861instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:35:56.741CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Isospin asymmetry in holographic baryonic matter
title Isospin asymmetry in holographic baryonic matter
spellingShingle Isospin asymmetry in holographic baryonic matter
Kovensky, Nicolas
Holographic QCD
QCD Phase Diagram
Isospin Asymmetry
Pion Condensation
title_short 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_sort Isospin asymmetry in holographic baryonic matter
dc.creator.none.fl_str_mv Kovensky, Nicolas
Schmitt, Andreas
author Kovensky, Nicolas
author_facet Kovensky, Nicolas
Schmitt, Andreas
author_role author
author2 Schmitt, Andreas
author2_role author
dc.subject.none.fl_str_mv Holographic QCD
QCD Phase Diagram
Isospin Asymmetry
Pion Condensation
topic Holographic QCD
QCD Phase Diagram
Isospin Asymmetry
Pion Condensation
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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.
Fil: Kovensky, Nicolas. Commissariat A L'energie Atomique. Institut de Recherche Des Lois Fondamentales de L'univers; Francia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Schmitt, Andreas. University of Southampton; Reino Unido
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.
publishDate 2021
dc.date.none.fl_str_mv 2021-07
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/255861
Kovensky, Nicolas; Schmitt, Andreas; Isospin asymmetry in holographic baryonic matter; SciPost Foundation; SciPost Physics; 11; 2; 7-2021; 029, 1-49
2542-4653
CONICET Digital
CONICET
url http://hdl.handle.net/11336/255861
identifier_str_mv Kovensky, Nicolas; Schmitt, Andreas; Isospin asymmetry in holographic baryonic matter; SciPost Foundation; SciPost Physics; 11; 2; 7-2021; 029, 1-49
2542-4653
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://scipost.org/SciPostPhys.11.2.029
info:eu-repo/semantics/altIdentifier/doi/10.21468/SciPostPhys.11.2.029
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv SciPost Foundation
publisher.none.fl_str_mv SciPost Foundation
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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