{"title":"扩展线性-西格玛模型:有限温度下 QCD 物质的输运特性","authors":"Adel Nasser Tawfik, Azzah Elshehri","doi":"10.1002/asna.20240004","DOIUrl":null,"url":null,"abstract":"<p>Since their discovery in heavy-ion collisions, the transport properties of quantum chromodynamics (QCD) matter gained prominence among nuclear theorists. We introduce a new study based on a QCD-like effective model. The thermal evolution of the electric and heat conductivity, <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>σ</mi>\n <mi>e</mi>\n </msub>\n </mrow>\n <annotation>$$ {\\sigma}_e $$</annotation>\n </semantics></math> and <span></span><math>\n <semantics>\n <mrow>\n <mi>κ</mi>\n </mrow>\n <annotation>$$ \\kappa $$</annotation>\n </semantics></math>, respectively, and that if their ratios are evaluated in SU(3) extended linear-sigma model (eLSM) with mean field approximation. Also, the bulk and shear viscosity normalized to the thermal entropy, <span></span><math>\n <semantics>\n <mrow>\n <mi>ξ</mi>\n <mo>/</mo>\n <mi>s</mi>\n </mrow>\n <annotation>$$ \\xi /s $$</annotation>\n </semantics></math> and <span></span><math>\n <semantics>\n <mrow>\n <mi>η</mi>\n <mo>/</mo>\n <mi>s</mi>\n </mrow>\n <annotation>$$ \\eta /s $$</annotation>\n </semantics></math>, respectively, as well as their ratios are estimated in the eLSM at finite temperature. Furthermore, the two ratios <span></span><math>\n <semantics>\n <mrow>\n <mrow>\n <mo>(</mo>\n <mrow>\n <mi>ξ</mi>\n <mo>/</mo>\n <mi>s</mi>\n </mrow>\n <mo>)</mo>\n </mrow>\n <mo>/</mo>\n <mfenced>\n <mrow>\n <msub>\n <mi>σ</mi>\n <mi>e</mi>\n </msub>\n <mspace></mspace>\n <mi>T</mi>\n </mrow>\n </mfenced>\n </mrow>\n <annotation>$$ \\left(\\xi /s\\right)/\\left({\\sigma}_e\\kern0.1em T\\right) $$</annotation>\n </semantics></math> and <span></span><math>\n <semantics>\n <mrow>\n <mrow>\n <mo>(</mo>\n <mrow>\n <mi>η</mi>\n <mo>/</mo>\n <mi>s</mi>\n </mrow>\n <mo>)</mo>\n </mrow>\n <mo>/</mo>\n <mfenced>\n <mrow>\n <msub>\n <mi>σ</mi>\n <mi>e</mi>\n </msub>\n <mspace></mspace>\n <mi>T</mi>\n </mrow>\n </mfenced>\n </mrow>\n <annotation>$$ \\left(\\eta /s\\right)/\\left({\\sigma}_e\\kern0.1em T\\right) $$</annotation>\n </semantics></math> are analyzed. The excellent agreement with recent lattice QCD calculations allows to draw the conclusion that the values assigned to the various eLSM-parameters make this QCD-like effective model capable of reproducing the non-perturbative calculations of QCD matter, at finite temperatures.</p>","PeriodicalId":55442,"journal":{"name":"Astronomische Nachrichten","volume":"345 2-3","pages":""},"PeriodicalIF":1.1000,"publicationDate":"2024-01-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Extended linear-sigma model: transport properties of QCD matter at finite temperature\",\"authors\":\"Adel Nasser Tawfik, Azzah Elshehri\",\"doi\":\"10.1002/asna.20240004\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Since their discovery in heavy-ion collisions, the transport properties of quantum chromodynamics (QCD) matter gained prominence among nuclear theorists. We introduce a new study based on a QCD-like effective model. The thermal evolution of the electric and heat conductivity, <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>σ</mi>\\n <mi>e</mi>\\n </msub>\\n </mrow>\\n <annotation>$$ {\\\\sigma}_e $$</annotation>\\n </semantics></math> and <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>κ</mi>\\n </mrow>\\n <annotation>$$ \\\\kappa $$</annotation>\\n </semantics></math>, respectively, and that if their ratios are evaluated in SU(3) extended linear-sigma model (eLSM) with mean field approximation. Also, the bulk and shear viscosity normalized to the thermal entropy, <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>ξ</mi>\\n <mo>/</mo>\\n <mi>s</mi>\\n </mrow>\\n <annotation>$$ \\\\xi /s $$</annotation>\\n </semantics></math> and <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>η</mi>\\n <mo>/</mo>\\n <mi>s</mi>\\n </mrow>\\n <annotation>$$ \\\\eta /s $$</annotation>\\n </semantics></math>, respectively, as well as their ratios are estimated in the eLSM at finite temperature. Furthermore, the two ratios <span></span><math>\\n <semantics>\\n <mrow>\\n <mrow>\\n <mo>(</mo>\\n <mrow>\\n <mi>ξ</mi>\\n <mo>/</mo>\\n <mi>s</mi>\\n </mrow>\\n <mo>)</mo>\\n </mrow>\\n <mo>/</mo>\\n <mfenced>\\n <mrow>\\n <msub>\\n <mi>σ</mi>\\n <mi>e</mi>\\n </msub>\\n <mspace></mspace>\\n <mi>T</mi>\\n </mrow>\\n </mfenced>\\n </mrow>\\n <annotation>$$ \\\\left(\\\\xi /s\\\\right)/\\\\left({\\\\sigma}_e\\\\kern0.1em T\\\\right) $$</annotation>\\n </semantics></math> and <span></span><math>\\n <semantics>\\n <mrow>\\n <mrow>\\n <mo>(</mo>\\n <mrow>\\n <mi>η</mi>\\n <mo>/</mo>\\n <mi>s</mi>\\n </mrow>\\n <mo>)</mo>\\n </mrow>\\n <mo>/</mo>\\n <mfenced>\\n <mrow>\\n <msub>\\n <mi>σ</mi>\\n <mi>e</mi>\\n </msub>\\n <mspace></mspace>\\n <mi>T</mi>\\n </mrow>\\n </mfenced>\\n </mrow>\\n <annotation>$$ \\\\left(\\\\eta /s\\\\right)/\\\\left({\\\\sigma}_e\\\\kern0.1em T\\\\right) $$</annotation>\\n </semantics></math> are analyzed. The excellent agreement with recent lattice QCD calculations allows to draw the conclusion that the values assigned to the various eLSM-parameters make this QCD-like effective model capable of reproducing the non-perturbative calculations of QCD matter, at finite temperatures.</p>\",\"PeriodicalId\":55442,\"journal\":{\"name\":\"Astronomische Nachrichten\",\"volume\":\"345 2-3\",\"pages\":\"\"},\"PeriodicalIF\":1.1000,\"publicationDate\":\"2024-01-18\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomische Nachrichten\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1002/asna.20240004\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomische Nachrichten","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/asna.20240004","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Extended linear-sigma model: transport properties of QCD matter at finite temperature
Since their discovery in heavy-ion collisions, the transport properties of quantum chromodynamics (QCD) matter gained prominence among nuclear theorists. We introduce a new study based on a QCD-like effective model. The thermal evolution of the electric and heat conductivity, and , respectively, and that if their ratios are evaluated in SU(3) extended linear-sigma model (eLSM) with mean field approximation. Also, the bulk and shear viscosity normalized to the thermal entropy, and , respectively, as well as their ratios are estimated in the eLSM at finite temperature. Furthermore, the two ratios and are analyzed. The excellent agreement with recent lattice QCD calculations allows to draw the conclusion that the values assigned to the various eLSM-parameters make this QCD-like effective model capable of reproducing the non-perturbative calculations of QCD matter, at finite temperatures.
期刊介绍:
Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.