{"title":"来自 IIB 型超引力的等离子体-等离子体三阶相变","authors":"Andrés Anabalón, Julio Oliva","doi":"10.1103/physrevlett.133.121601","DOIUrl":null,"url":null,"abstract":"We show that the planar, charged black hole in asymptotically anti–de Sitter spacetime, dual to the strongly coupled quark-gluon plasma thermal state of large <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>N</mi></math>, <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>SU</mi></mrow><mo stretchy=\"false\">(</mo><mi>N</mi><mo stretchy=\"false\">)</mo></math>, <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi mathvariant=\"script\">N</mi><mo>=</mo><mn>4</mn></math> super Yang-Mills at finite chemical potential undergoes a third-order phase transition in the grand canonical ensemble to a hairy black hole of type IIB supergravity. The hairy phase is another strongly coupled fluid with a conformal equation of state and can be interpreted as another kind of quark-gluon plasma. This new quark-gluon plasma has less entropy and, therefore, seems to characterize some form of smooth hadronization. The locus of the transition in terms of the critical values of the “baryon” chemical potential <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>μ</mi><mi>c</mi></msub></math> and the temperature <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>T</mi><mi>c</mi></msub></math> is <math display=\"inline\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>μ</mi><mi>c</mi></msub><mo>=</mo><mn>2</mn><mi>π</mi><msub><mi>T</mi><mi>c</mi></msub></math>.","PeriodicalId":20069,"journal":{"name":"Physical review letters","volume":null,"pages":null},"PeriodicalIF":8.1000,"publicationDate":"2024-09-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Plasma-Plasma Third Order Phase Transition from Type IIB Supergravity\",\"authors\":\"Andrés Anabalón, Julio Oliva\",\"doi\":\"10.1103/physrevlett.133.121601\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We show that the planar, charged black hole in asymptotically anti–de Sitter spacetime, dual to the strongly coupled quark-gluon plasma thermal state of large <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>N</mi></math>, <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mi>SU</mi></mrow><mo stretchy=\\\"false\\\">(</mo><mi>N</mi><mo stretchy=\\\"false\\\">)</mo></math>, <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi mathvariant=\\\"script\\\">N</mi><mo>=</mo><mn>4</mn></math> super Yang-Mills at finite chemical potential undergoes a third-order phase transition in the grand canonical ensemble to a hairy black hole of type IIB supergravity. The hairy phase is another strongly coupled fluid with a conformal equation of state and can be interpreted as another kind of quark-gluon plasma. This new quark-gluon plasma has less entropy and, therefore, seems to characterize some form of smooth hadronization. The locus of the transition in terms of the critical values of the “baryon” chemical potential <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>μ</mi><mi>c</mi></msub></math> and the temperature <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>T</mi><mi>c</mi></msub></math> is <math display=\\\"inline\\\" xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>μ</mi><mi>c</mi></msub><mo>=</mo><mn>2</mn><mi>π</mi><msub><mi>T</mi><mi>c</mi></msub></math>.\",\"PeriodicalId\":20069,\"journal\":{\"name\":\"Physical review letters\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":8.1000,\"publicationDate\":\"2024-09-19\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physical review letters\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1103/physrevlett.133.121601\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical review letters","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevlett.133.121601","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
Plasma-Plasma Third Order Phase Transition from Type IIB Supergravity
We show that the planar, charged black hole in asymptotically anti–de Sitter spacetime, dual to the strongly coupled quark-gluon plasma thermal state of large , , super Yang-Mills at finite chemical potential undergoes a third-order phase transition in the grand canonical ensemble to a hairy black hole of type IIB supergravity. The hairy phase is another strongly coupled fluid with a conformal equation of state and can be interpreted as another kind of quark-gluon plasma. This new quark-gluon plasma has less entropy and, therefore, seems to characterize some form of smooth hadronization. The locus of the transition in terms of the critical values of the “baryon” chemical potential and the temperature is .
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