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Local truncation residual for the θ heat scheme
Statement
Let , , , , , , and . Let , , and suppose satisfies
u_t-\kappa_xu_{xx}-\kappa_yu_{yy}=f$$ on $\overline\Omega\times[0,T]$, with exact sampled initial and Dirichlet rows in the scheme of [Fully discrete θ heat finite-difference scheme](/item/def-parabolic-theta-finite-difference-scheme). Assume $u_{tt},u_{ttt},u_{xxxx},u_{yyyy}$ are continuous on the closed cylinder, and write $M_{tt},M_{ttt},M_{x4},M_{y4}$ for their respective sup norms there. If $r^n$ is the exact grid sample at time $t_n$, the complete interior residual is bounded at every time step by|\tau^n|\infty\le \Delta t M{tt}+\frac{\kappa_xh_x^2M_{x4}+\kappa_yh_y^2M_{y4}}{12}\quad(\theta\ne\tfrac12),
|\tau^n|\infty\le\frac{(\Delta t)^2M{ttt}}{12}+\frac{\kappa_xh_x^2M_{x4}+\kappa_yh_y^2M_{y4}}{12}\quad(\theta=\tfrac12),
where $\tau^n$ is defined by substituting the exact samples and the exact boundary rows into the fully discrete equation, including its interior rows adjacent to the boundary.Facts & Assumptions
Given: The rectangular domain and finite mesh above; ; ; an exact solution with the stated continuous derivatives satisfying ; and exact initial and boundary samples.
Fully discrete θ heat finite-difference scheme defines the centered heat stencil, the endpoint-weighted source , and boundary contributions from both endpoint rows.
Proof
At each interior node set and define , where and applies the centered stencil using that exact boundary row. Applying the PDE at and rewrites this as the weighted average of the two spatial stencil defects plus .
For a one-variable function , Taylor expansion at an interior node gives for some and . Thus the absolute error is at most . The stencil uses the exact boundary samples at the first and last interior rows, so the same Taylor estimate applies there. Applying it in and bounds each spatial defect in step 1.1 by .
Put . The quotient is the average of on the time interval. For , both this average and lie between the minimum and maximum of on that interval; their difference is therefore at most its oscillation, which is at most . For , let be the linear interpolant of at the two endpoints. The interpolation remainder satisfies . Integrating and dividing by gives . These are the required bounds for the temporal term in step 1.1.
Combining the two spatial bounds from step 2.1 with the temporal bound from step 2.2 in the residual identity of step 1.1 gives the two asserted estimates at every interior node. Taking the maximum over nodes and time steps proves the stated complete-residual bounds.
Remarks
The derivatives are assumed up to the closed space-time boundary, so the proof includes boundary-adjacent interior rows. Exact boundary samples are essential; no result for a lower-order or different boundary closure is asserted. No choice axiom is used.
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Sources
- Endre Süli, B6.1 Numerical Solution of Partial Differential Equations: A brief introduction to the theory of finite difference approximation of PDEs (standard reference, not scraped)
- Benjamin Seibold, MIT 18.336, Lecture 14: Von Neumann Stability Analysis (Spring 2009) (standard reference, not scraped)
- Martin Krosche, Hermann G. Matthies, and Oliver Kayser-Herold, Lecture Notes: Introduction to PDEs and Numerical Methods, Technical University Braunschweig, Revision 1.1 (2008), hosted by University of Jyväskylä (standard reference, not scraped)