Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model
In this paper we explore independently for the first time three chemical potentials (baryon $\mu_B$, charged $\mu_Q$, and strange $\mu_S$) in the Chiral mean-field (CMF) model. We designed and implemented \texttt{CMF++}, a new version of the CMF model rewritten in \texttt{C++} that is optimized, mod...
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creator | Cruz-Camacho, Nikolas Kumar, Rajesh Pelicer, Mateus Reinke Peterson, Jeff Manning, T. Andrew Haas, Roland Dexheimer, Veronica Noronha-Hostler, Jaquelyn |
description | In this paper we explore independently for the first time three chemical
potentials (baryon $\mu_B$, charged $\mu_Q$, and strange $\mu_S$) in the Chiral
mean-field (CMF) model. We designed and implemented \texttt{CMF++}, a new
version of the CMF model rewritten in \texttt{C++} that is optimized, modular,
and well-documented. \texttt{CMF++} has been integrated into the MUSES
Calculation Engine as a free and open source software module. The runtime
improved in more than 4 orders of magnitude across all 3 chemical potentials,
when compared to the legacy code. Here we focus on the zero temperature case
and study stable, as well as metastable and unstable, vacuum, hadronic, and
quark phases, showing how phase boundaries vary with the different chemical
potentials. Due to the significant numerical improvements in \texttt{CMF++}, we
can calculate for the first time high-order susceptibilities within the CMF
framework to study the properties of the quark deconfinement phase transition.
We found phases of matter that include a light hadronic phase,
strangeness-dominated hadronic phase, and quark deconfinement within our
$\mu_B$, $\mu_S$, $\mu_Q$ phase space. The phase transitions are of first,
second (quantum critical point), and third order between these phases and we
even identified a tricritical point. |
doi_str_mv | 10.48550/arxiv.2409.06837 |
format | Article |
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potentials (baryon $\mu_B$, charged $\mu_Q$, and strange $\mu_S$) in the Chiral
mean-field (CMF) model. We designed and implemented \texttt{CMF++}, a new
version of the CMF model rewritten in \texttt{C++} that is optimized, modular,
and well-documented. \texttt{CMF++} has been integrated into the MUSES
Calculation Engine as a free and open source software module. The runtime
improved in more than 4 orders of magnitude across all 3 chemical potentials,
when compared to the legacy code. Here we focus on the zero temperature case
and study stable, as well as metastable and unstable, vacuum, hadronic, and
quark phases, showing how phase boundaries vary with the different chemical
potentials. Due to the significant numerical improvements in \texttt{CMF++}, we
can calculate for the first time high-order susceptibilities within the CMF
framework to study the properties of the quark deconfinement phase transition.
We found phases of matter that include a light hadronic phase,
strangeness-dominated hadronic phase, and quark deconfinement within our
$\mu_B$, $\mu_S$, $\mu_Q$ phase space. The phase transitions are of first,
second (quantum critical point), and third order between these phases and we
even identified a tricritical point.</description><identifier>DOI: 10.48550/arxiv.2409.06837</identifier><language>eng</language><subject>Physics - High Energy Astrophysical Phenomena ; Physics - High Energy Physics - Phenomenology ; Physics - Nuclear Theory</subject><creationdate>2024-09</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2409.06837$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2409.06837$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Cruz-Camacho, Nikolas</creatorcontrib><creatorcontrib>Kumar, Rajesh</creatorcontrib><creatorcontrib>Pelicer, Mateus Reinke</creatorcontrib><creatorcontrib>Peterson, Jeff</creatorcontrib><creatorcontrib>Manning, T. Andrew</creatorcontrib><creatorcontrib>Haas, Roland</creatorcontrib><creatorcontrib>Dexheimer, Veronica</creatorcontrib><creatorcontrib>Noronha-Hostler, Jaquelyn</creatorcontrib><title>Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model</title><description>In this paper we explore independently for the first time three chemical
potentials (baryon $\mu_B$, charged $\mu_Q$, and strange $\mu_S$) in the Chiral
mean-field (CMF) model. We designed and implemented \texttt{CMF++}, a new
version of the CMF model rewritten in \texttt{C++} that is optimized, modular,
and well-documented. \texttt{CMF++} has been integrated into the MUSES
Calculation Engine as a free and open source software module. The runtime
improved in more than 4 orders of magnitude across all 3 chemical potentials,
when compared to the legacy code. Here we focus on the zero temperature case
and study stable, as well as metastable and unstable, vacuum, hadronic, and
quark phases, showing how phase boundaries vary with the different chemical
potentials. Due to the significant numerical improvements in \texttt{CMF++}, we
can calculate for the first time high-order susceptibilities within the CMF
framework to study the properties of the quark deconfinement phase transition.
We found phases of matter that include a light hadronic phase,
strangeness-dominated hadronic phase, and quark deconfinement within our
$\mu_B$, $\mu_S$, $\mu_Q$ phase space. The phase transitions are of first,
second (quantum critical point), and third order between these phases and we
even identified a tricritical point.</description><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Physics - Nuclear Theory</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNqFjrEOgjAUALs4GPUDnHw_UKwCijNqXIwm6kye8ggvKS1p0cjfi8Td6Ya74YSYLlQQJXGs5uje_AqWkdoEapWE66G4nUv0BJcG76y5aYENNCVBKLdckfFsDWo41WSkt0_3IEhtTlBY12dpya7zFaGRBZPO4dhpPRaDArWnyY8jMdvvrulB9gNZ7bhC12bfkawfCf8XH8UJPVg</recordid><startdate>20240910</startdate><enddate>20240910</enddate><creator>Cruz-Camacho, Nikolas</creator><creator>Kumar, Rajesh</creator><creator>Pelicer, Mateus Reinke</creator><creator>Peterson, Jeff</creator><creator>Manning, T. Andrew</creator><creator>Haas, Roland</creator><creator>Dexheimer, Veronica</creator><creator>Noronha-Hostler, Jaquelyn</creator><scope>GOX</scope></search><sort><creationdate>20240910</creationdate><title>Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model</title><author>Cruz-Camacho, Nikolas ; Kumar, Rajesh ; Pelicer, Mateus Reinke ; Peterson, Jeff ; Manning, T. Andrew ; Haas, Roland ; Dexheimer, Veronica ; Noronha-Hostler, Jaquelyn</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_2409_068373</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - High Energy Physics - Phenomenology</topic><topic>Physics - Nuclear Theory</topic><toplevel>online_resources</toplevel><creatorcontrib>Cruz-Camacho, Nikolas</creatorcontrib><creatorcontrib>Kumar, Rajesh</creatorcontrib><creatorcontrib>Pelicer, Mateus Reinke</creatorcontrib><creatorcontrib>Peterson, Jeff</creatorcontrib><creatorcontrib>Manning, T. Andrew</creatorcontrib><creatorcontrib>Haas, Roland</creatorcontrib><creatorcontrib>Dexheimer, Veronica</creatorcontrib><creatorcontrib>Noronha-Hostler, Jaquelyn</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Cruz-Camacho, Nikolas</au><au>Kumar, Rajesh</au><au>Pelicer, Mateus Reinke</au><au>Peterson, Jeff</au><au>Manning, T. Andrew</au><au>Haas, Roland</au><au>Dexheimer, Veronica</au><au>Noronha-Hostler, Jaquelyn</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model</atitle><date>2024-09-10</date><risdate>2024</risdate><abstract>In this paper we explore independently for the first time three chemical
potentials (baryon $\mu_B$, charged $\mu_Q$, and strange $\mu_S$) in the Chiral
mean-field (CMF) model. We designed and implemented \texttt{CMF++}, a new
version of the CMF model rewritten in \texttt{C++} that is optimized, modular,
and well-documented. \texttt{CMF++} has been integrated into the MUSES
Calculation Engine as a free and open source software module. The runtime
improved in more than 4 orders of magnitude across all 3 chemical potentials,
when compared to the legacy code. Here we focus on the zero temperature case
and study stable, as well as metastable and unstable, vacuum, hadronic, and
quark phases, showing how phase boundaries vary with the different chemical
potentials. Due to the significant numerical improvements in \texttt{CMF++}, we
can calculate for the first time high-order susceptibilities within the CMF
framework to study the properties of the quark deconfinement phase transition.
We found phases of matter that include a light hadronic phase,
strangeness-dominated hadronic phase, and quark deconfinement within our
$\mu_B$, $\mu_S$, $\mu_Q$ phase space. The phase transitions are of first,
second (quantum critical point), and third order between these phases and we
even identified a tricritical point.</abstract><doi>10.48550/arxiv.2409.06837</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Phenomenology Physics - Nuclear Theory |
title | Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model |
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