Space-time virtual elements for the heat equation
Sergio Gómez, Lorenzo Mascotto, Andrea Moiola, Ilaria Perugia
TL;DR
The paper develops a space-time virtual element method for the heat equation on a space-time cylinder $Q_T$, using local VE spaces that solve heat problems with polynomial data and nonconforming global spaces linked by upwind projections. It establishes well-posedness through a VE Newton potential and a discrete inf-sup condition, and proves optimal a priori error estimates under isotropic mesh assumptions. Numerical results in $(1+1)$ and $(2+1)$ dimensions validate the theoretical rates, show robustness to incompatible data, and demonstrate high-order convergence with increasing degree $p$ or hp-adaptivity potential. The method offers a flexible, high-order framework on general prismatic space-time meshes, enabling time-slab decomposition, potential Trefftz variants, and adaptive refinement without dimension-dependent constraints.
Abstract
We propose and analyze a space-time virtual element method for the discretization of the heat equation in a space-time cylinder, based on a standard Petrov-Galerkin formulation. Local discrete functions are solutions to a heat equation problem with polynomial data. Global virtual element spaces are nonconforming in space, so that the analysis and the design of the method are independent of the spatial dimension. The information between time slabs is transmitted by means of upwind terms involving polynomial projections of the discrete functions. We prove well posedness and optimal error estimates for the scheme, and validate them with several numerical tests.
