2020
DOI: 10.1007/s10114-020-9367-4
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Convergence Rate for Galerkin Approximation of the Stochastic Allen—Cahn Equations on 2D Torus

Abstract: In this paper we discuss the convergence rate for Galerkin approximation of the stochastic Allen-Cahn equations driven by space-time white noise on T 2 . First we prove that the convergence rate for stochastic 2D heat equation is of order α − δ in Besov space C −α for α ∈ (0, 1) and δ > 0 arbitrarily small. Then we obtain the convergence rate for Galerkin approximation of the stochastic Allen-Cahn equations of order α − δ in C −α for α ∈ (0, 2/9) and δ > 0 arbitrarily small.

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Cited by 2 publications
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“…Considering the solutions as elements of distributional spaces is necessary in higher dimensional versions of the stochastic Allen-Cahn equations, also known as the dynamical Φ 4 d models, which for this reason have to be renormalised. The dependence of the rate of convergence of approximations on the choice of the Besov exponent is observed in [MZ20], where the authors consider the spatial semidiscretisation of Φ 4 2 and bound the B −θ ∞,∞ norm of the error by n −θ+ε for any ε > 0, under the constraint θ ∈ (0, 2/9). In [HM18,ZZ18] the convergence of spatial semidiscretisations of Φ 4…”
Section: Resultsmentioning
confidence: 99%
“…Considering the solutions as elements of distributional spaces is necessary in higher dimensional versions of the stochastic Allen-Cahn equations, also known as the dynamical Φ 4 d models, which for this reason have to be renormalised. The dependence of the rate of convergence of approximations on the choice of the Besov exponent is observed in [MZ20], where the authors consider the spatial semidiscretisation of Φ 4 2 and bound the B −θ ∞,∞ norm of the error by n −θ+ε for any ε > 0, under the constraint θ ∈ (0, 2/9). In [HM18,ZZ18] the convergence of spatial semidiscretisations of Φ 4…”
Section: Resultsmentioning
confidence: 99%