2015
DOI: 10.1515/cmam-2015-0026
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Space-Time Finite Element Methods for Parabolic Problems

Abstract: We propose and analyze a space-time finite element method for the numerical solution of parabolic evolution equations. This approach allows the use of general and unstructured space-time finite elements which do not require any tensor product structure. The stability of the numerical scheme is based on a stability condition which holds for standard finite element spaces. We also provide related a priori error estimates which are confirmed by numerical experiments.

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Cited by 102 publications
(104 citation statements)
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(28 reference statements)
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“…Recently, a space–time finite‐element method has been analyzed by Steinbach for solving the Dirichlet boundary value problem for the heat equation, as follows: αtufalse(x,tfalse)Δxufalse(x,tfalse)=ffalse(x,tfalse)1emfor2.56804ptfalse(x,tfalse)Q:=normalΩ×false(0,Tfalse), with given boundary and initial conditions, that is, u ( x , t )=0 for ( x , t )∈Σ:= ∂ Ω×(0, T ), and u ( x ,0)= u 0 ( x ) for x ∈Ω, respectively. Here, normalΩRn, and therefore, QRn+1, n =2,3, is a bounded Lipschitz domain, and αR+ is the heat capacity constant.…”
Section: Adaptive Space–time Finite‐element Methodsmentioning
confidence: 99%
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“…Recently, a space–time finite‐element method has been analyzed by Steinbach for solving the Dirichlet boundary value problem for the heat equation, as follows: αtufalse(x,tfalse)Δxufalse(x,tfalse)=ffalse(x,tfalse)1emfor2.56804ptfalse(x,tfalse)Q:=normalΩ×false(0,Tfalse), with given boundary and initial conditions, that is, u ( x , t )=0 for ( x , t )∈Σ:= ∂ Ω×(0, T ), and u ( x ,0)= u 0 ( x ) for x ∈Ω, respectively. Here, normalΩRn, and therefore, QRn+1, n =2,3, is a bounded Lipschitz domain, and αR+ is the heat capacity constant.…”
Section: Adaptive Space–time Finite‐element Methodsmentioning
confidence: 99%
“…The related discrete Galerkin–Petrov variational formulation is to find uhXhX such that afalse(uh,vhfalse)=0.1emf,vhafalse(u0,vhfalse) is satisfied for all vhYhY, where we assume XhYh. A standard stability and error analysis for the space–time finite‐element method was concluded from a discrete inf‐sup condition, as shown in the work by Steinbach . In particular, the space–time cylinder Q is decomposed into admissible and shape regular finite elements q ℓ , that is, Qh==1Ntrueq¯.…”
Section: Adaptive Space–time Finite‐element Methodsmentioning
confidence: 99%
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