2019
DOI: 10.3934/cpaa.2019056
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Backward compact and periodic random attractors for non-autonomous sine-Gordon equations with multiplicative noise

Abstract: A non-autonomous random attractor is called backward compact if its backward union is pre-compact. We show that such a backward compact random attractor exists if a non-autonomous random dynamical system is bounded dissipative and backward asymptotically compact. We also obtain both backward compact and periodic random attractor from a periodic and locally asymptotically compact system. The abstract results are applied to the sine-Gordon equation with multiplicative noise and a time-dependent force. If we assu… Show more

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Cited by 15 publications
(11 citation statements)
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“…This means φ is backward asymptotically compact in V g (O) (see [12]). Therefore, our result follows from an abstract result on bi-spatial random attractor given in [15] and [17] immediately.…”
supporting
confidence: 59%
See 2 more Smart Citations
“…This means φ is backward asymptotically compact in V g (O) (see [12]). Therefore, our result follows from an abstract result on bi-spatial random attractor given in [15] and [17] immediately.…”
supporting
confidence: 59%
“…Some abstract theoretical criteria were established in [6,16,25,26] for deterministic cases and [17] for stochastic ones. In order to establish the existence result of a backward compact random attractor in H g (O), where H g (O) is a special subspace of the weighted space L 2 g (O) 2 , we assume that the force f is backward tempered and the so-called backward asymptotic compactness, which indicates that the usual asymptotic compactness is uniform in the past, is introduced.…”
Section: 3)mentioning
confidence: 99%
See 1 more Smart Citation
“…A schematic illustration of the dislocation mechanisms operative in different length scale regimes is given in Figure . With decreasing layer thickness starting in the micron range the dominant deformation mechanisms change from dislocation pile‐up to confined layer slip (CLS) of dislocations (<50 nm) and finally to interface crossing of dislocations (slip transfer) (<2.5 nm) leading to strain localization that limits the uniform deformability . These mechanisms may be transferred to ARB by considering the peculiarities of interface‐mediated plasticity.…”
Section: Selected Arb Systemsmentioning
confidence: 99%
“…We must prove that the random dynamical system (or cocycle) is backward asymptotically compact in X , which means that the pullback asymptotic compactness is uniform in the past. By combining the bounded backward absorption, we need to establish the backward compactness [10][11][12][13][14] of the PRA  , which means that ∪ s≤  (s, ) is relatively compact in X . The backward compactness in X is available via the Ascoli-Arzelà theorem and it often leads to the longtime stability of the PRA in X as in (1).…”
Section: Introductionmentioning
confidence: 99%