A scalar finite-volume update is monotone if increasing any input state cannot decrease any output state. A consistent conservative update preserves constants and has an invariant interval by comparison. On a periodic grid, or an infinite grid with summable perturbations, conservation and monotonicity imply L1 contraction of a monotone conservative scheme. Translation invariance then implies the total variation diminishing scheme property.
A translation-invariant conservative monotone update decreases discrete total variation. If is the one-cell shift, , and L1 contraction of a monotone conservative scheme applied to gives . This prevents creation of new total variation, though it does not make every discontinuity sharply resolved.
Let be a monotone conservative scalar update on a periodic grid. Since , one has . Conservation makes the sum of the right side equal to . Reverse and add to obtain . On an infinite grid the same proof holds for summable differences with a Lipschitz flux on the state range.
The Engquist-Osher method is the finite volume method using the Engquist-Osher flux. Under on the invariant state interval, its update is monotone. It preserves the state range, is contractive for summable perturbations in , and decreases discrete total variation.
Monotonicity of the explicit update requires on its invariant state interval. Convexity and a unique sonic point of a scalar flux do not remove this time-step restriction. For , linearization about a positive constant gives an upwind finite difference scheme for advection equation: , where . At Fourier frequency the multiplier is , whose modulus exceeds one when . Thus a CFL condition is essential to the claimed nonlinear stability.
The Engquist-Osher numerical flux is . It sends positive-speed contributions from the left state and negative-speed contributions from the right state. Its consistency and opposite monotonicities in the two arguments yield a monotone conservative scheme under the appropriate Courant–Friedrichs–Lewy condition. For the Inviscid Burgers equation, it is .
For a flux that is a differentiable convex function with unique minimum at , define for and zero otherwise, and for and zero otherwise. The Engquist-Osher flux is . Thus transsonic rarefaction wave states give , while reversed transsonic states give . This follows by integrating the positive and negative parts of .
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