{ "id": "1602.07262", "version": "v1", "published": "2016-02-23T18:45:59.000Z", "updated": "2016-02-23T18:45:59.000Z", "title": "Intermittency fronts for space-time fractional stochastic partial differential equations in $(d+1)$ dimensions", "authors": [ "Sunday A. Asogwa", "Erkan Nane" ], "comment": "17 pages, submitted for publication. arXiv admin note: substantial text overlap with arXiv:1409.7468", "categories": [ "math.PR", "math-ph", "math.AP", "math.MP" ], "abstract": "We consider time fractional stochastic heat type equation $$\\partial^\\beta_tu_t(x)=-\\nu(-\\Delta)^{\\alpha/2} u_t(x)+I^{1-\\beta}_t[\\sigma(u)\\stackrel{\\cdot}{W}(t,x)]$$ in $(d+1)$ dimensions, where $\\nu>0$, $\\beta\\in (0,1)$, $\\alpha\\in (0,2]$, $d<\\min\\{2,\\beta^{-1}\\}\\a$, $\\partial^\\beta_t$ is the Caputo fractional derivative, $-(-\\Delta)^{\\alpha/2} $ is the generator of an isotropic stable process, $\\stackrel{\\cdot}{W}(t,x)$ is space-time white noise, and $\\sigma:\\R \\to\\RR{R}$ is Lipschitz continuous. Mijena and Nane proved in \\cite{JebesaAndNane1} that : (i) absolute moments of the solutions of this equation grows exponentially; and (ii) the distances to the origin of the farthest high peaks of those moments grow exactly linearly with time. The last result was proved under the assumptions $\\alpha=2$ and $d=1.$ In this paper we extend this result to the case $\\alpha=2$ and $d\\in\\{1,2,3\\}.$", "revisions": [ { "version": "v1", "updated": "2016-02-23T18:45:59.000Z" } ], "analyses": { "subjects": [ "60H15" ], "keywords": [ "space-time fractional stochastic partial differential", "fractional stochastic partial differential equations", "intermittency fronts", "fractional stochastic heat type", "stochastic heat type equation" ], "note": { "typesetting": "TeX", "pages": 17, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016arXiv160207262A" } } }