{"title":"由乘法时空白噪声驱动的随机时分数布尔格斯方程的$L_p$$$可解性和霍尔德正则性","authors":"Beom-Seok Han","doi":"10.1007/s40072-024-00329-w","DOIUrl":null,"url":null,"abstract":"<p>This paper establishes <span>\\(L_p\\)</span>-solvability for stochastic time fractional Burgers’ equations driven by multiplicative space-time white noise: </p><span>$$\\begin{aligned} \\partial _t^\\alpha u = a^{ij}u_{x^ix^j} + b^{i}u_{x^i} + cu + {\\bar{b}}^i u u_{x^i} + \\partial _t^\\beta \\int _0^t \\sigma (u)dW_t,\\quad t>0;\\quad u(0,\\cdot ) = u_0, \\end{aligned}$$</span><p>where <span>\\(\\alpha \\in (0,1)\\)</span>, <span>\\(\\beta < 3\\alpha /4+1/2\\)</span>, and <span>\\(d< 4--2(2\\beta -1)_+/\\alpha \\)</span>. The operators <span>\\(\\partial _t^\\alpha \\)</span> and <span>\\(\\partial _t^\\beta \\)</span> are the Caputo fractional derivatives of order <span>\\(\\alpha \\)</span> and <span>\\(\\beta \\)</span>, respectively. The process <span>\\(W_t\\)</span> is an <span>\\(L_2(\\mathbb {R}^d)\\)</span>-valued cylindrical Wiener process, and the coefficients <span>\\(a^{ij}, b^i, c, {\\bar{b}}^{i}\\)</span> and <span>\\(\\sigma (u)\\)</span> are random. In addition to the uniqueness and existence of a solution, the Hölder regularity of the solution is also established. For example, for any constant <span>\\(T<\\infty \\)</span>, small <span>\\(\\varepsilon >0\\)</span>, and almost sure <span>\\(\\omega \\in \\varOmega \\)</span>, </p><span>$$\\begin{aligned} \\sup _{x\\in \\mathbb {R}^d}|u(\\omega ,\\cdot ,x)|_{C^{\\left[ \\frac{\\alpha }{2}\\left( \\left( 2-(2\\beta -1)_+/\\alpha -d/2 \\right) \\wedge 1 \\right) +\\frac{(2\\beta -1)_{-}}{2} \\right] \\wedge 1-\\varepsilon }([0,T])}<\\infty \\end{aligned}$$</span><p>and </p><span>$$\\begin{aligned} \\sup _{t\\le T}|u(\\omega ,t,\\cdot )|_{C^{\\left( 2-(2\\beta -1)_+/\\alpha -d/2 \\right) \\wedge 1 - \\varepsilon }(\\mathbb {R}^d)} < \\infty . \\end{aligned}$$</span><p>The Hölder regularity of the solution in time changes behavior at <span>\\(\\beta = 1/2\\)</span>. Furthermore, if <span>\\(\\beta \\ge 1/2\\)</span>, then the Hölder regularity of the solution in time is <span>\\(\\alpha /2\\)</span> times that in space.</p>","PeriodicalId":48569,"journal":{"name":"Stochastics and Partial Differential Equations-Analysis and Computations","volume":null,"pages":null},"PeriodicalIF":1.4000,"publicationDate":"2024-04-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"$$L_p$$ -solvability and Hölder regularity for stochastic time fractional Burgers’ equations driven by multiplicative space-time white noise\",\"authors\":\"Beom-Seok Han\",\"doi\":\"10.1007/s40072-024-00329-w\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>This paper establishes <span>\\\\(L_p\\\\)</span>-solvability for stochastic time fractional Burgers’ equations driven by multiplicative space-time white noise: </p><span>$$\\\\begin{aligned} \\\\partial _t^\\\\alpha u = a^{ij}u_{x^ix^j} + b^{i}u_{x^i} + cu + {\\\\bar{b}}^i u u_{x^i} + \\\\partial _t^\\\\beta \\\\int _0^t \\\\sigma (u)dW_t,\\\\quad t>0;\\\\quad u(0,\\\\cdot ) = u_0, \\\\end{aligned}$$</span><p>where <span>\\\\(\\\\alpha \\\\in (0,1)\\\\)</span>, <span>\\\\(\\\\beta < 3\\\\alpha /4+1/2\\\\)</span>, and <span>\\\\(d< 4--2(2\\\\beta -1)_+/\\\\alpha \\\\)</span>. The operators <span>\\\\(\\\\partial _t^\\\\alpha \\\\)</span> and <span>\\\\(\\\\partial _t^\\\\beta \\\\)</span> are the Caputo fractional derivatives of order <span>\\\\(\\\\alpha \\\\)</span> and <span>\\\\(\\\\beta \\\\)</span>, respectively. The process <span>\\\\(W_t\\\\)</span> is an <span>\\\\(L_2(\\\\mathbb {R}^d)\\\\)</span>-valued cylindrical Wiener process, and the coefficients <span>\\\\(a^{ij}, b^i, c, {\\\\bar{b}}^{i}\\\\)</span> and <span>\\\\(\\\\sigma (u)\\\\)</span> are random. In addition to the uniqueness and existence of a solution, the Hölder regularity of the solution is also established. For example, for any constant <span>\\\\(T<\\\\infty \\\\)</span>, small <span>\\\\(\\\\varepsilon >0\\\\)</span>, and almost sure <span>\\\\(\\\\omega \\\\in \\\\varOmega \\\\)</span>, </p><span>$$\\\\begin{aligned} \\\\sup _{x\\\\in \\\\mathbb {R}^d}|u(\\\\omega ,\\\\cdot ,x)|_{C^{\\\\left[ \\\\frac{\\\\alpha }{2}\\\\left( \\\\left( 2-(2\\\\beta -1)_+/\\\\alpha -d/2 \\\\right) \\\\wedge 1 \\\\right) +\\\\frac{(2\\\\beta -1)_{-}}{2} \\\\right] \\\\wedge 1-\\\\varepsilon }([0,T])}<\\\\infty \\\\end{aligned}$$</span><p>and </p><span>$$\\\\begin{aligned} \\\\sup _{t\\\\le T}|u(\\\\omega ,t,\\\\cdot )|_{C^{\\\\left( 2-(2\\\\beta -1)_+/\\\\alpha -d/2 \\\\right) \\\\wedge 1 - \\\\varepsilon }(\\\\mathbb {R}^d)} < \\\\infty . \\\\end{aligned}$$</span><p>The Hölder regularity of the solution in time changes behavior at <span>\\\\(\\\\beta = 1/2\\\\)</span>. Furthermore, if <span>\\\\(\\\\beta \\\\ge 1/2\\\\)</span>, then the Hölder regularity of the solution in time is <span>\\\\(\\\\alpha /2\\\\)</span> times that in space.</p>\",\"PeriodicalId\":48569,\"journal\":{\"name\":\"Stochastics and Partial Differential Equations-Analysis and Computations\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":1.4000,\"publicationDate\":\"2024-04-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Stochastics and Partial Differential Equations-Analysis and Computations\",\"FirstCategoryId\":\"100\",\"ListUrlMain\":\"https://doi.org/10.1007/s40072-024-00329-w\",\"RegionNum\":3,\"RegionCategory\":\"数学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"MATHEMATICS, APPLIED\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Stochastics and Partial Differential Equations-Analysis and Computations","FirstCategoryId":"100","ListUrlMain":"https://doi.org/10.1007/s40072-024-00329-w","RegionNum":3,"RegionCategory":"数学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"MATHEMATICS, APPLIED","Score":null,"Total":0}
$$L_p$$ -solvability and Hölder regularity for stochastic time fractional Burgers’ equations driven by multiplicative space-time white noise
This paper establishes \(L_p\)-solvability for stochastic time fractional Burgers’ equations driven by multiplicative space-time white noise:
$$\begin{aligned} \partial _t^\alpha u = a^{ij}u_{x^ix^j} + b^{i}u_{x^i} + cu + {\bar{b}}^i u u_{x^i} + \partial _t^\beta \int _0^t \sigma (u)dW_t,\quad t>0;\quad u(0,\cdot ) = u_0, \end{aligned}$$
where \(\alpha \in (0,1)\), \(\beta < 3\alpha /4+1/2\), and \(d< 4--2(2\beta -1)_+/\alpha \). The operators \(\partial _t^\alpha \) and \(\partial _t^\beta \) are the Caputo fractional derivatives of order \(\alpha \) and \(\beta \), respectively. The process \(W_t\) is an \(L_2(\mathbb {R}^d)\)-valued cylindrical Wiener process, and the coefficients \(a^{ij}, b^i, c, {\bar{b}}^{i}\) and \(\sigma (u)\) are random. In addition to the uniqueness and existence of a solution, the Hölder regularity of the solution is also established. For example, for any constant \(T<\infty \), small \(\varepsilon >0\), and almost sure \(\omega \in \varOmega \),
The Hölder regularity of the solution in time changes behavior at \(\beta = 1/2\). Furthermore, if \(\beta \ge 1/2\), then the Hölder regularity of the solution in time is \(\alpha /2\) times that in space.
期刊介绍:
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