{"title":"IP矩阵模型中的Krylov复杂度","authors":"Norihiro Iizuka, Mitsuhiro Nishida","doi":"10.1007/jhep11(2023)065","DOIUrl":null,"url":null,"abstract":"A bstract The IP matrix model is a simple large N quantum mechanical model made up of an adjoint harmonic oscillator plus a fundamental harmonic oscillator. It is a model introduced previously as a toy model of the gauge theory dual of an AdS black hole. In the large N limit, one can solve the Schwinger-Dyson equation for the fundamental correlator, and at sufficiently high temperature, this model shows key signatures of thermalization and information loss; the correlator decay exponentially in time, and the spectral density becomes continuous and gapless. We study the Lanczos coefficients b n in this model and at sufficiently high temperature, it grows linearly in n with logarithmic corrections, which is one of the fastest growth under certain conditions. As a result, the Krylov complexity grows exponentially in time as $$ \\sim \\exp \\left(\\mathcal{O}\\left(\\sqrt{t}\\right)\\right) $$ <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\"> <mml:mo>∼</mml:mo> <mml:mo>exp</mml:mo> <mml:mfenced> <mml:mrow> <mml:mi>O</mml:mi> <mml:mfenced> <mml:msqrt> <mml:mi>t</mml:mi> </mml:msqrt> </mml:mfenced> </mml:mrow> </mml:mfenced> </mml:math> . These results indicate that the IP model at sufficiently high temperature is chaotic.","PeriodicalId":48906,"journal":{"name":"Journal of High Energy Physics","volume":" 772","pages":"0"},"PeriodicalIF":5.0000,"publicationDate":"2023-11-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"9","resultStr":"{\"title\":\"Krylov complexity in the IP matrix model\",\"authors\":\"Norihiro Iizuka, Mitsuhiro Nishida\",\"doi\":\"10.1007/jhep11(2023)065\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A bstract The IP matrix model is a simple large N quantum mechanical model made up of an adjoint harmonic oscillator plus a fundamental harmonic oscillator. It is a model introduced previously as a toy model of the gauge theory dual of an AdS black hole. In the large N limit, one can solve the Schwinger-Dyson equation for the fundamental correlator, and at sufficiently high temperature, this model shows key signatures of thermalization and information loss; the correlator decay exponentially in time, and the spectral density becomes continuous and gapless. We study the Lanczos coefficients b n in this model and at sufficiently high temperature, it grows linearly in n with logarithmic corrections, which is one of the fastest growth under certain conditions. As a result, the Krylov complexity grows exponentially in time as $$ \\\\sim \\\\exp \\\\left(\\\\mathcal{O}\\\\left(\\\\sqrt{t}\\\\right)\\\\right) $$ <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\"> <mml:mo>∼</mml:mo> <mml:mo>exp</mml:mo> <mml:mfenced> <mml:mrow> <mml:mi>O</mml:mi> <mml:mfenced> <mml:msqrt> <mml:mi>t</mml:mi> </mml:msqrt> </mml:mfenced> </mml:mrow> </mml:mfenced> </mml:math> . These results indicate that the IP model at sufficiently high temperature is chaotic.\",\"PeriodicalId\":48906,\"journal\":{\"name\":\"Journal of High Energy Physics\",\"volume\":\" 772\",\"pages\":\"0\"},\"PeriodicalIF\":5.0000,\"publicationDate\":\"2023-11-10\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"9\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of High Energy Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1007/jhep11(2023)065\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, PARTICLES & FIELDS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of High Energy Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1007/jhep11(2023)065","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 9
摘要
IP矩阵模型是一个简单的大N量子力学模型,由一个伴随谐振子和一个基谐振子组成。这是一个以前作为标准理论对偶黑洞的玩具模型介绍的模型。在大N极限下,可以求解基本相关器的Schwinger-Dyson方程,并且在足够高的温度下,该模型显示出热化和信息损失的关键特征;相关器随时间呈指数衰减,谱密度变为连续无间隙。我们在该模型中研究了Lanczos系数bn,在足够高的温度下,它随n的对数修正线性增长,是在一定条件下增长最快的一种。因此,Krylov复杂度随时间呈指数增长,为$$ \sim \exp \left(\mathcal{O}\left(\sqrt{t}\right)\right) $$ ~ exp O t。这些结果表明,在足够高的温度下,IP模型是混沌的。
A bstract The IP matrix model is a simple large N quantum mechanical model made up of an adjoint harmonic oscillator plus a fundamental harmonic oscillator. It is a model introduced previously as a toy model of the gauge theory dual of an AdS black hole. In the large N limit, one can solve the Schwinger-Dyson equation for the fundamental correlator, and at sufficiently high temperature, this model shows key signatures of thermalization and information loss; the correlator decay exponentially in time, and the spectral density becomes continuous and gapless. We study the Lanczos coefficients b n in this model and at sufficiently high temperature, it grows linearly in n with logarithmic corrections, which is one of the fastest growth under certain conditions. As a result, the Krylov complexity grows exponentially in time as $$ \sim \exp \left(\mathcal{O}\left(\sqrt{t}\right)\right) $$ ∼expOt . These results indicate that the IP model at sufficiently high temperature is chaotic.
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