2020
DOI: 10.1007/s10543-020-00807-2
|View full text |Cite
|
Sign up to set email alerts
|

Lower and upper bounds for strong approximation errors for numerical approximations of stochastic heat equations

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
2

Citation Types

0
5
0

Year Published

2022
2022
2024
2024

Publication Types

Select...
4
1

Relationship

1
4

Authors

Journals

citations
Cited by 5 publications
(5 citation statements)
references
References 17 publications
0
5
0
Order By: Relevance
“…Comparing (1.4) with the sharp temporal Hölder continuity result in Theorem 2.6, one can easily observe, for γ ∈ ( d 2 , 2], the rate of convergence is in accordance with the temporal Hölder continuity of the mild solution. For γ ∈ [2,4], the rate of the convergence can reach 1 and higher than the Hölder continuity of the mild solution. It must be emphasized that the derivation of (1.4) is not an easy task and requires a variety of delicate error estimates, which are elaborated in subsection 3.3.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…Comparing (1.4) with the sharp temporal Hölder continuity result in Theorem 2.6, one can easily observe, for γ ∈ ( d 2 , 2], the rate of convergence is in accordance with the temporal Hölder continuity of the mild solution. For γ ∈ [2,4], the rate of the convergence can reach 1 and higher than the Hölder continuity of the mild solution. It must be emphasized that the derivation of (1.4) is not an easy task and requires a variety of delicate error estimates, which are elaborated in subsection 3.3.…”
Section: Introductionmentioning
confidence: 99%
“…As indicated in [2], the fully discrete exponential Euler and fully discrete linear-implicit Euler approximations diverge strongly and numerically weakly in the case of stochastic Allen-Cahn equations. Later, some explicit modified Euler-type schemes have been proposed in [3,4,5,9,19,28] to numerically solve the stochastic Allen-Cahn equations. Based on a spectral Galerkin spatial approximation of (1.1), given by dX N (t) + A(AX N (t) + P N F (X N (t)))dt = P N dW (t), t ∈ (0, T ]; X N (0) = P N X 0 ,…”
Section: Introductionmentioning
confidence: 99%
“…This shows that for all N ∈ N we have that N 3 realizations of standard normal random variables are used to calculate one realization of X N 2 ,N T . Combining (6) with the computational effort N 3 illustrates that for all ε ∈ (0, 1 /6) we have that the approximation scheme in (2)-( 3) converges with the overall rate 1 /6 − ε with respect to the number of used independent standard normal random variables.…”
Section: Thenmentioning
confidence: 94%
“…Next we would like to point out that the numerical approximation scheme (3) has been proposed in Hutzenthaler et al [21] and has there been referred to as a nonlinearity-truncated approximation scheme (cf. [21, (3) in Section 1] and, e.g., [17][18][19][20]24,25,35,36,38,40] for further research articles on explicit approximation schemes for stochastic differential equations with superlinearly growing nonlinearities).…”
Section: Thenmentioning
confidence: 99%
See 1 more Smart Citation