1986
DOI: 10.1214/aop/1176992360
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Isotropic Stochastic Flows

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Cited by 91 publications
(120 citation statements)
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“…We note that in the case where inertia of the particles can be neglected, our results reduce to calculating the Lyapunov exponent for a spatially correlated Brownian motion, which was discussed from a mathematical point of view by Le Jan (1985) and Baxendale & Harris (1986).…”
Section: Illustration and Contextmentioning
confidence: 89%
“…We note that in the case where inertia of the particles can be neglected, our results reduce to calculating the Lyapunov exponent for a spatially correlated Brownian motion, which was discussed from a mathematical point of view by Le Jan (1985) and Baxendale & Harris (1986).…”
Section: Illustration and Contextmentioning
confidence: 89%
“…Its positivity w as established in 8 for velocity elds that are a nite-dimensional Ornstein-Uhlenbeck process. The Jacobian and the evolution of curves in isotropic stochastic ows with zero drift is studied in 4 . The trajectories of 1.1 behave v ery di erently from mean zero time dependent ows.…”
Section: Evolution Of the Jacobian Matrixmentioning
confidence: 99%
“…In particular we should have that E ffYt; yg E ffSt; yg We note further that the generator 10.2 is formally of the form L J f = c J ; J @ 2 f @J@J : 10.6 Such di usion processes have t ypically positive non-zero Lyapunov exponents, that is, the limit = lim T!1 lnjjJtjj T exists with probability one, and 0. The computation of for some time dependent o ws was done in 4,8,31,19,20 . We shall show in Section 11 that in our case = 0.…”
Section: Evolution Of the Jacobian Matrixmentioning
confidence: 99%
“…Although extensive literature is available for stochastic flows driven by standard Brownian motion (see [5,13]), very little is known when the driver of the flow is changed to a nonMarkovian, non-diffusive process, such as fractional Brownian motion. For instance, some of the very basic results concerning the tangent flow are yet to be unearthed in the case when the flow is driven by fractional Brownian motion.…”
Section: Introductionmentioning
confidence: 99%
“…To this end, note first that from (14) we can bound the second integrand by |D 1−α t− B H γ,t− (r)| ≤ k 1 (α, β) B H γ β,T (t − r) α+β−1 . Now using (5) and Assumptions (A2)-(A4), the first integrand can be bounded by…”
mentioning
confidence: 99%