{"title":"芬斯勒时空上的最优传输和时间性下里奇曲率边界","authors":"Mathias Braun, Shin-ichi Ohta","doi":"10.1090/tran/9126","DOIUrl":null,"url":null,"abstract":"<p>We prove that a Finsler spacetime endowed with a smooth reference measure whose induced weighted Ricci curvature <inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"normal upper R normal i normal c Subscript upper N\"> <mml:semantics> <mml:msub> <mml:mrow> <mml:mi mathvariant=\"normal\">R</mml:mi> <mml:mi mathvariant=\"normal\">i</mml:mi> <mml:mi mathvariant=\"normal\">c</mml:mi> </mml:mrow> <mml:mi>N</mml:mi> </mml:msub> <mml:annotation encoding=\"application/x-tex\">\\mathrm {Ric}_N</mml:annotation> </mml:semantics> </mml:math> </inline-formula> is bounded from below by a real number <inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"upper K\"> <mml:semantics> <mml:mi>K</mml:mi> <mml:annotation encoding=\"application/x-tex\">K</mml:annotation> </mml:semantics> </mml:math> </inline-formula> in every timelike direction satisfies the timelike curvature-dimension condition <inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"normal upper T normal upper C normal upper D Subscript q Baseline left-parenthesis upper K comma upper N right-parenthesis\"> <mml:semantics> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=\"normal\">T</mml:mi> <mml:mi mathvariant=\"normal\">C</mml:mi> <mml:mi mathvariant=\"normal\">D</mml:mi> </mml:mrow> <mml:mi>q</mml:mi> </mml:msub> <mml:mo stretchy=\"false\">(</mml:mo> <mml:mi>K</mml:mi> <mml:mo>,</mml:mo> <mml:mi>N</mml:mi> <mml:mo stretchy=\"false\">)</mml:mo> </mml:mrow> <mml:annotation encoding=\"application/x-tex\">\\mathrm {TCD}_q(K,N)</mml:annotation> </mml:semantics> </mml:math> </inline-formula> for all <inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"q element-of left-parenthesis 0 comma 1 right-parenthesis\"> <mml:semantics> <mml:mrow> <mml:mi>q</mml:mi> <mml:mo>∈<!-- ∈ --></mml:mo> <mml:mo stretchy=\"false\">(</mml:mo> <mml:mn>0</mml:mn> <mml:mo>,</mml:mo> <mml:mn>1</mml:mn> <mml:mo stretchy=\"false\">)</mml:mo> </mml:mrow> <mml:annotation encoding=\"application/x-tex\">q\\in (0,1)</mml:annotation> </mml:semantics> </mml:math> </inline-formula>. The converse and a nonpositive-dimensional version (<inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"upper N less-than-or-equal-to 0\"> <mml:semantics> <mml:mrow> <mml:mi>N</mml:mi> <mml:mo>≤<!-- ≤ --></mml:mo> <mml:mn>0</mml:mn> </mml:mrow> <mml:annotation encoding=\"application/x-tex\">N \\le 0</mml:annotation> </mml:semantics> </mml:math> </inline-formula>) of this result are also shown. Our discussion is based on the solvability of the Monge problem with respect to the <inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"q\"> <mml:semantics> <mml:mi>q</mml:mi> <mml:annotation encoding=\"application/x-tex\">q</mml:annotation> </mml:semantics> </mml:math> </inline-formula>-Lorentz–Wasserstein distance as well as the characterization of <inline-formula content-type=\"math/mathml\"> <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" alttext=\"q\"> <mml:semantics> <mml:mi>q</mml:mi> <mml:annotation encoding=\"application/x-tex\">q</mml:annotation> </mml:semantics> </mml:math> </inline-formula>-geodesics of probability measures. One consequence of our work is the sharp timelike Brunn–Minkowski inequality in the Lorentz–Finsler case.</p>","PeriodicalId":23209,"journal":{"name":"Transactions of the American Mathematical Society","volume":"36 1","pages":""},"PeriodicalIF":1.2000,"publicationDate":"2024-02-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Optimal transport and timelike lower Ricci curvature bounds on Finsler spacetimes\",\"authors\":\"Mathias Braun, Shin-ichi Ohta\",\"doi\":\"10.1090/tran/9126\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>We prove that a Finsler spacetime endowed with a smooth reference measure whose induced weighted Ricci curvature <inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"normal upper R normal i normal c Subscript upper N\\\"> <mml:semantics> <mml:msub> <mml:mrow> <mml:mi mathvariant=\\\"normal\\\">R</mml:mi> <mml:mi mathvariant=\\\"normal\\\">i</mml:mi> <mml:mi mathvariant=\\\"normal\\\">c</mml:mi> </mml:mrow> <mml:mi>N</mml:mi> </mml:msub> <mml:annotation encoding=\\\"application/x-tex\\\">\\\\mathrm {Ric}_N</mml:annotation> </mml:semantics> </mml:math> </inline-formula> is bounded from below by a real number <inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"upper K\\\"> <mml:semantics> <mml:mi>K</mml:mi> <mml:annotation encoding=\\\"application/x-tex\\\">K</mml:annotation> </mml:semantics> </mml:math> </inline-formula> in every timelike direction satisfies the timelike curvature-dimension condition <inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"normal upper T normal upper C normal upper D Subscript q Baseline left-parenthesis upper K comma upper N right-parenthesis\\\"> <mml:semantics> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=\\\"normal\\\">T</mml:mi> <mml:mi mathvariant=\\\"normal\\\">C</mml:mi> <mml:mi mathvariant=\\\"normal\\\">D</mml:mi> </mml:mrow> <mml:mi>q</mml:mi> </mml:msub> <mml:mo stretchy=\\\"false\\\">(</mml:mo> <mml:mi>K</mml:mi> <mml:mo>,</mml:mo> <mml:mi>N</mml:mi> <mml:mo stretchy=\\\"false\\\">)</mml:mo> </mml:mrow> <mml:annotation encoding=\\\"application/x-tex\\\">\\\\mathrm {TCD}_q(K,N)</mml:annotation> </mml:semantics> </mml:math> </inline-formula> for all <inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"q element-of left-parenthesis 0 comma 1 right-parenthesis\\\"> <mml:semantics> <mml:mrow> <mml:mi>q</mml:mi> <mml:mo>∈<!-- ∈ --></mml:mo> <mml:mo stretchy=\\\"false\\\">(</mml:mo> <mml:mn>0</mml:mn> <mml:mo>,</mml:mo> <mml:mn>1</mml:mn> <mml:mo stretchy=\\\"false\\\">)</mml:mo> </mml:mrow> <mml:annotation encoding=\\\"application/x-tex\\\">q\\\\in (0,1)</mml:annotation> </mml:semantics> </mml:math> </inline-formula>. The converse and a nonpositive-dimensional version (<inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"upper N less-than-or-equal-to 0\\\"> <mml:semantics> <mml:mrow> <mml:mi>N</mml:mi> <mml:mo>≤<!-- ≤ --></mml:mo> <mml:mn>0</mml:mn> </mml:mrow> <mml:annotation encoding=\\\"application/x-tex\\\">N \\\\le 0</mml:annotation> </mml:semantics> </mml:math> </inline-formula>) of this result are also shown. Our discussion is based on the solvability of the Monge problem with respect to the <inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"q\\\"> <mml:semantics> <mml:mi>q</mml:mi> <mml:annotation encoding=\\\"application/x-tex\\\">q</mml:annotation> </mml:semantics> </mml:math> </inline-formula>-Lorentz–Wasserstein distance as well as the characterization of <inline-formula content-type=\\\"math/mathml\\\"> <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" alttext=\\\"q\\\"> <mml:semantics> <mml:mi>q</mml:mi> <mml:annotation encoding=\\\"application/x-tex\\\">q</mml:annotation> </mml:semantics> </mml:math> </inline-formula>-geodesics of probability measures. One consequence of our work is the sharp timelike Brunn–Minkowski inequality in the Lorentz–Finsler case.</p>\",\"PeriodicalId\":23209,\"journal\":{\"name\":\"Transactions of the American Mathematical Society\",\"volume\":\"36 1\",\"pages\":\"\"},\"PeriodicalIF\":1.2000,\"publicationDate\":\"2024-02-26\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Transactions of the American Mathematical Society\",\"FirstCategoryId\":\"100\",\"ListUrlMain\":\"https://doi.org/10.1090/tran/9126\",\"RegionNum\":2,\"RegionCategory\":\"数学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"MATHEMATICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Transactions of the American Mathematical Society","FirstCategoryId":"100","ListUrlMain":"https://doi.org/10.1090/tran/9126","RegionNum":2,"RegionCategory":"数学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"MATHEMATICS","Score":null,"Total":0}
引用次数: 0
摘要
我们证明了一个赋有光滑参考量度的芬斯勒时空,其诱导加权里奇曲率 R i c N \mathrm {Ric}_N 在每个时间方向上自下而上被实数 K K 限定,满足所有 q∈ ( 0 , 1 ) q\in (0,1) 的时间曲率维度条件 T C D q ( K , N ) \mathrm {TCD}_q(K,N) 。这个结果的反面和非正维版本 ( N ≤ 0 N \le 0 ) 也被展示出来。我们的讨论基于 Monge 问题关于 q q -Lorentz-Wasserstein 距离的可解性以及概率测度的 q q -geodesics 的特征。我们工作的一个结果是洛伦兹-芬斯勒情况下的尖锐时间状布伦-闵科夫斯基不等式。
Optimal transport and timelike lower Ricci curvature bounds on Finsler spacetimes
We prove that a Finsler spacetime endowed with a smooth reference measure whose induced weighted Ricci curvature RicN\mathrm {Ric}_N is bounded from below by a real number KK in every timelike direction satisfies the timelike curvature-dimension condition TCDq(K,N)\mathrm {TCD}_q(K,N) for all q∈(0,1)q\in (0,1). The converse and a nonpositive-dimensional version (N≤0N \le 0) of this result are also shown. Our discussion is based on the solvability of the Monge problem with respect to the qq-Lorentz–Wasserstein distance as well as the characterization of qq-geodesics of probability measures. One consequence of our work is the sharp timelike Brunn–Minkowski inequality in the Lorentz–Finsler case.
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