Inviscid Burgers equation Created 2026-09-24 Updated 2026-10-14
The Inviscid Burgers equation is the scalar conservation lawFor a classical solution, the chain rule makes this equivalent to , a nonlinear transport equation with characteristic speed . The conservative form remains meaningful for a discontinuous weak solution, whereas the product cannot simply be evaluated pointwise at a jump. Its discontinuities obey the Rankine-Hugoniot condition ; this condition alone permits inadmissible expansion jumps. For bounded initial conditions on the infinite line, imposing the Kruzhkov entropy inequalities and the initial trace selects a unique entropy solution. For step data, incoming characteristic curves select , while produces a rarefaction wave.[ref]
Past exam of the mathematics course of the University of Cambridge 2006 iii Paper 68 6 Solution Created 2026-10-03 Updated 2026-10-14
The Engquist-Osher method is an upwind finite volume method. For cell values , mesh width and time step , put and use the conservative updatewhere the numerical flux isConsistency of a numerical method follows from . Positive characteristic speeds use the left state, and negative speeds use the right state. The flux difference telescopes when summed over cells, giving a discrete conservation law. The method is first order in space and time for smooth solutions; its conservation law form is also appropriate when shock waves develop.
Let be the unique sonic point of a scalar flux, . Convexity implies to its left and to its right. Put and splitThen , , , andThis is the sonic-point splitting of a convex Engquist-Osher flux. If both states are above , ; if both are below it, . Across a transsonic rarefaction wave, , the flux is the minimum . In the opposite crossing it is , which in general differs from the exact Godunov numerical flux. This distinction does not affect the monotonicity proof.
Here stability requires the usual Courant–Friedrichs–Lewy condition. Let the initial values lie in , and chooseA differentiable convex function has a continuous derivative on this interval, so the maximum is finite. Write the three-input update as . Differentiating givesThus the update preserves componentwise order. Constants are fixed, since , so comparison with the constants proves for every time level. In particular the same CFL condition remains applicable. This is a mesh-independent maximum-principle stability bound.
A stronger stability statement is contraction in discrete . Consider two solutions in the same invariant interval, on a periodic mesh or on the infinite lattice with summable differences. Let be their componentwise maximum. Monotonicity gives , henceThe discrete conservation law for the difference gives the equality: on a finite periodic mesh the flux sum cancels exactly, and on the infinite lattice it follows by truncation and the fact that the flux is a Lipschitz function on . Interchanging and adding provesThis is L1 contraction of a monotone conservative scheme. Since commutes with the cell shift, applying this contraction to and its shift gives . The scheme is therefore a total variation diminishing scheme as well.
The same order argument proves a discrete entropy inequality, explaining why this stable discretization selects entropy solutions rather than nonphysical expansion shock waves. For a constant , setBecause and , their componentwise difference is at least . Subtracting their updates givesFor constants outside , the entropy inequality is an equality by the invariant bound and the conservative update. At equal states , the Kruzhkov entropy flux. The flux is a Lipschitz function on the invariant interval: writing , the conservative update gives . This time-translation bound, the invariant bound and the total variation estimate give local space-time compactness for bounded-variation initial conditions as the mesh is refined; the conservative update passes to the weak conservation law, and the displayed inequality passes to its Kruzhkov entropy inequality. This identifies the limit as the entropy solution.
Finally the time-step qualification is essential. For the convex Inviscid Burgers equation flux , whose unique sonic point of a scalar flux is zero, linearize about a positive constant . The perturbation update becomes . At Fourier frequency its multiplier is , with modulus greater than one if . Wave packets near this phase give linear instability even for summable Cauchy perturbations. Thus the assumptions on imply the stability results above under the CFL condition, not for arbitrary . This is CFL necessity for explicit Engquist-Osher stability.
Viscous Burgers equation Created 2026-09-29 Updated 2026-10-14
The viscous Burgers equation combines a nonlinear transport equation with diffusion with constant . On the infinite line, a bounded initial condition gives a smooth function solving the equation for every positive time; a jump in the initial condition is smoothed rather than retained as a discontinuity. Small can nevertheless produce a steep layer, as the Viscous Burgers travelling shock illustrates. The Cole-Hopf transformation , with positive , converts this equation to the heat equation .[ref]
Positive diffusion also explains the admissibility of the inviscid limit. For the entropy flux for a scalar conservation law associated with , direct multiplication by givesThe last term is nonpositive. With convergence sufficient to pass to the limit, the vanishing viscosity approximation therefore retains an entropy inequality rather than just the weak solution equation. For general bounded data, the full Kruzhkov entropy inequalities specify the entropy solution; the quadratic identity is a useful illustration of dissipation.[ref]