For positive smooth tube area , the equation becomes under the displayed transformation. Indeed, cancels geometrical spreading and makes the remaining nonlinear and transport coefficients equal. Starting with gives and ; characteristic crossing first occurs when , if that supremum is positive.
Before characteristic crossing, the method of characteristics for the Inviscid Burgers equation transports each initial value without changing it:
Here labels the starting position. Suppose is a bounded continuously differentiable function with bounded derivative. As long as for every label, the characteristic flow map is invertible and differentiating it gives the displayed formula for .[ref]
If the negative minimum is attained, the first breaking time is . Two labels with have formal intersection time
Their neighboring-label limit explains why the most negative initial slope breaks first. As , the amplitude remains bounded but diverges: this is gradient blow-up. Continuing intersecting lines would assign incompatible values at one position; the post-breaking entropy solution instead uses shock waves. Nondecreasing data have no forward characteristic crossing by this mechanism.
For a concrete calculation in dimensionless quantities on the infinite line, choose , with limiting states and . Then has minimum at , so and the breaking point is . Along the central characteristic curve , and before breaking. The labels give intersecting formal lines at , after the classical solution has already broken.
Figure 1.
Decreasing initial data steepen: the first gradient blow-up is at time 1, before two selected characteristics intersect
. Details.
Before characteristic crossing, the scalar conservation law has solution with . When this map is a diffeomorphism, the solution is . Its spatial derivative is .
Putting and transforms into the scalar conservation law
Along smooth characteristic curves, is constant and grows at speed . Starting from gives
After characteristic crossing, the Rankine-Hugoniot condition and entropy solution select the physical front.
Use material coordinates and write the placement as . The strain energy density in the printed convention is per unit reference mass. It is convenient to use the conventional first Piola-Kirchhoff stress tensor , so
Assume the undeformed reference state is stress-free. With and infinitesimal strain tensor , material isotropy and material frame indifference give the quadratic expansion
Consequently the Lamé parameters from hyperelastic energy Hessian are
Indeed, differentiating the quadratic expression twice gives
the elastic stiffness tensor of linear elasticity. A prestressed reference state requires the corresponding initial-stress corrections; the displayed formula concerns the natural state.
For a plane elastic wave, , put and . Balance of momentum without body force becomes
This is a material-coordinate equation: the reference density cancels between inertia and nominal stress. If , the first-order system has characteristic speeds and right eigenvectors . Along a characteristic curve with , its differential compatibility relation is
This follows by multiplying the system by the left eigenvector . It does not assert the existence of globally integrable Riemann invariants for an arbitrary three-component constitutive law.
There is a necessary qualification to the finite-amplitude transverse request. Set and , so . The longitudinal momentum equation requires
Thus arbitrary nonuniform pure transverse profiles are possible only if the compatibility condition for pure nonlinear transverse waves holds:
The third component vanishes by the reflection symmetry implied by isotropy and objectivity. The shear equation then closes:
General compressible hyperelastic material assumptions alone do not imply the required compatibility. For a concrete counterexample, take the Saint Venant–Kirchhoff hyperelastic energy
For , this becomes
At , . A varying shear therefore produces a longitudinal force and cannot preserve . Infinitesimal transverse waves do exist, because this coupling is second order, but a general pure finite-amplitude transverse wave does not.
The compatible nonlinear shear energy class is nonempty and can be genuinely nonlinear. Define , , and, for , take
This is objective and isotropic. Near , , so it has the specified Lamé parameters. On the plane deformation above, and . Hence at , while
For positive , the relevant incremental plane moduli are positive. This supplies an explicit stable pure transverse family and, when , amplitude-dependent wave speed.
For any compatible family, let
The equations and give the Riemann invariants
Consider the initially undisturbed half-space . A right-going simple wave has the incoming invariant , so . Denote the prescribed boundary nominal stress by . The physical boundary traction, whose outward normal is , is . Invert the monotone law to obtain . The wave state emitted at boundary time is transported along
Ahead of the leading front the state is zero. Before characteristic crossing, these equations determine the unique emission time for each disturbed point. The displacement itself is also determined, rather than just its derivatives:
Differentiating the implicit emission relation verifies and , so this is the complete pre-shock simple wave solution.
Write . The boundary-generated characteristic curves lose invertibility when
Thus the characteristic crossing in a boundary-generated elastic simple wave criterion is
Here . A smoothly increasing boundary stress therefore steepens into a shock wave only when later states travel faster: . Increasing stress alone is insufficient. For the compatible example with and , , so a nonzero increasing ramp produces finite-time crossing. For all rays are parallel and no such shock forms. This criterion locates the first gradient singularity; subsequent discontinuous evolution additionally requires the jump conditions and an admissibility condition.
For a general vector simple wave, replace the pure-shear line by an integral curve
Substitution gives , with the same emission construction and crossing criterion. Boundary tractions must lie on this one-family curve. Generic finite-amplitude quasi-transverse waves may contain longitudinal displacement; arbitrary vector boundary forcing need not generate a single simple wave.
On a region with smooth positive area, set , . Substitution into the simple wave equation gives
Remove the last term by , and choose . Starting at a regular section , one convenient normalized area transformation of a nonlinear acoustic simple wave is
In the notation , set . The remaining equation is . With initial value at , the method of characteristics gives
The map from the initial label loses invertibility when . For smooth data with bounded derivative and , the first forward characteristic crossing is at ; if , no forward shock occurs.
For spherical spreading, write physical radius as and specify data at an emitting radius . Since ,
The shock distance for a spherical simple wave launched at finite radius is
If the axial distance is measured from the emitting surface, , then and
No finite shock distance exists in this model when .
The printed combination with general bounded data at is singular and does not define the intended outgoing spherical initial-value problem. Along a spherical characteristic, and , so is constant. A bounded trace at forces that constant to be zero for every characteristic curve emanating from the origin; arbitrary nonzero bounded cannot be launched there. For example, the ostensibly admissible data would demand both and a nonzero trace, a contradiction. The logarithmic transformed distance is also divergent at the origin. Thus an unqualified numerical shock formula from those literal data would be unjustified. The finite-radius formulas above give the physical interpretation once the launching radius, or the shifted area law, is supplied.
For , , so the characteristic speed is and the conservation law flux is strictly convex. Let and let be the initial vertical position of a characteristic curve.
For the increasing ramp, the characteristic curves within its sloping part satisfy . They spread apart and never cross. The outer plateau characteristic speeds are and , so the complete entropy solution is
The transition widens linearly and its gradient decreases. At large time it approaches a rarefaction wave, with inside its expanding transition.
For the decreasing ramp, and the characteristic curves converge. Before they meet,
All the ramp characteristic curves meet at at
Thereafter a stationary sedimentation shock separates below from above. Indeed the Rankine-Hugoniot condition gives
and the incoming characteristic speeds satisfy , which makes it an admissible entropy shock. The discontinuity transports no net excess particle flux because both plateau fluxes equal . These are local solutions before a finite container's boundaries affect the transition.
Figure 1.
Spreading and shock formation for quadratic hindered-settling flux
. Details.
The dependence on is controlled by the hindered-settling flux inflection:
For any smooth initial profile, the characteristic flow map has derivative
This formula gives the first characteristic crossing: minimize the positive values of . At neither ramp changes shape; both move down at . For , the flux is convex throughout : the increasing ramp spreads and the decreasing ramp steepens, although its entire ramp generally no longer focuses simultaneously. For , the flux is concave throughout that interval and these roles reverse. At the endpoint values the curvature vanishes at one plateau; it does not reverse sign inside the interval.
For , the inflection lies between the plateau concentrations. Below the increasing ramp spreads, while above it that ramp compresses; the decreasing ramp has the opposite local behavior. After characteristic crossing, the entropy solution can contain both a shock wave and a rarefaction wave. Quantitatively, an increasing step is selected by the lower convex envelope of on the interval between its states: curved portions supply rarefaction waves, and straight portions supply shock waves. A decreasing step uses the upper concave envelope. A join between a fan and a shock wave at a state satisfies the tangent-chord relation , where is the other shock state. Thus curvature, not simply the magnitude of , decides the wave pattern; the envelope may reduce to one shock if the tangent lies outside the state interval.
For the negative-flux Inviscid Burgers equation, the method of characteristics gives
The characteristic curve starting at therefore has , and hence
For smooth data this describes a single-valued classical solution as long as the characteristic flow map is invertible. Its Jacobian is ; after characteristic crossing, one must instead select a weak solution with the appropriate entropy solution condition.
The conservation form is , with conservation law flux . Integrating this scalar conservation law across a moving discontinuity, or differentiating its Heaviside representation as a distribution, yields the Rankine-Hugoniot condition
For distinct one-sided limits it simplifies to
This jump-speed relation is exact for the Burgers conservation law; an additional entropy condition is needed to distinguish a physical compressive shock wave from an expansion discontinuity.
The step gives the Burgers Riemann problem with negative flux. If , characteristic curves from the left have speed zero, while those from the right have speed : they converge. The entropy shock wave has speed and thus
Characteristics enter this shock from both sides, since .
If , the right-hand speed is positive and the two families separate. A smooth steep approximation to the initial step spreads into a rarefaction wave. In the fan, the self-similar characteristic curve relation is , giving
The endpoint values match continuously. The discontinuity moving at would satisfy the jump condition even for , but its characteristic curves leave the discontinuity and it fails entropy admissibility. For the solution is identically zero.
Figure 1.
Characteristics of the negative-flux Burgers step: compression gives a shock for positive U, while negative U gives a rarefaction fan
. Details.
For the sharp energy estimate, stays uniform while the available bound diverges as when . If the coarser estimate is used for the first part, both displayed bounds diverge, but the first divergence is only an artifact of discarding an exact cancellation.
The method of characteristics explains why uniform control of the gradient cannot generally persist for the inviscid scalar conservation law. Before characteristic crossing, with initial data ,
If somewhere, the denominator reaches zero in finite positive time. The solution steepens and the smooth description breaks down; an entropy solution can subsequently contain shocks. Positive viscosity replaces such a discontinuity by a thin smooth layer, which can have large gradient even while its norm remains controlled. The divergent bound does not assert that every flux and every initial datum form a shock; a linear flux, for example, has no such steepening.
Write the negative-flux Inviscid Burgers equation as , with . Along a characteristic curve,
so a characteristic starting at has and
This formula is a classical solution only while the method of characteristics is one-to-one; after characteristic crossing one must select an entropy solution.
For a discontinuity with left and right values and , the Rankine-Hugoniot condition follows by integrating conservation across a moving small interval:
For a nonzero jump, factor the difference of squares to obtain
The negative flux makes increasing jumps compressive. Decreasing jumps spread into rarefaction waves; they cannot be retained as nonphysical expansion shock waves.
In the central ramp of each period, , so its method of characteristics is . For , the retained ramp therefore occupies . At the odd boundary , the initial limiting values are on the left and on the right. Their characteristic speeds are and , giving the fan on . Together these give the periodic backward-sawtooth Burgers solution
These intervals tile the real line up to their matching endpoints, where both formulas agree at . The increasing ramp steepens, but the wave's maximum magnitude remains one before breaking. A steep continuous regularization of the original downward jump produces exactly the limiting fan, as suggested by the characteristic construction.
At , each increasing ramp collapses at . The fans on either side meet there with values and , producing a compressive stationary shock wave. For all the fan between successive shock waves remains centered at the odd point, giving
At a shock wave the limiting values are and . Their average is zero, so the Rankine-Hugoniot condition keeps the shock wave fixed. Their characteristic speeds satisfy , confirming compression into the shock wave. The arbitrary pointwise value at a shock wave does not affect the weak solution. The post-breaking amplitude decays as , despite the lack of explicit viscosity, because shock wave dissipate the wave.
For the requested sketches, has ramp slope on and fan slope around odd points on width . It is still continuous. At , the profile decreases linearly with slope between even points and jumps from to at each even point:
Figure 1.
Periodic Burgers wave before breaking at Z equals one third and after breaking at Z equals three, with stationary shocks at even theta
. Details.
Write . Since , choosing gives and . At the maximizing foot , the inverse-flux quadratic bounds give
Combining the two estimates and dividing by gives
The last step uses and the sign-independent bound on . This is square-root decay before characteristic crossing; it is proved only for . No continuation past characteristic crossing or global-time smoothness is assumed. If , the initial function and the solution vanish.
When the velocity depends on , different initial values travel at different speeds. The resulting characteristic crossing can destroy a classical solution in finite time, even though the initial function is smooth and bounded. For the Inviscid Burgers equation, take . Before crossing,
and
At this tends to as , while . Thus The bounded-derivative Burgers flux agrees with this equation on the whole state range, if a global bounded-speed flux is desired. After crossing, arbitrary weak solutions need not be unique; an entropy solution condition is needed to select the admissible continuation.
Now the mass per unit radius satisfies the nonlinear scalar conservation law
Its characteristic curves have speed
Because and increases with , the high central part of a localized pulse travels inward faster than its low-density edges. On the inner, rising side, faster high-density characteristics catch slower low-density ones, causing characteristic crossing and an inward-facing shock wave. On the outer, falling side, the characteristics separate and form a rarefaction wave. The initial bump therefore develops a sharp inner front and a broad outer tail while moving toward the star.
Set
The scalar conservation law is . Its characteristic curve issuing from satisfies
The Jacobian of the one-dimensional characteristic map is
Before characteristic crossing, differentiation with respect to gives
Because has compact support, is continuous and vanishes outside a compact set. It therefore attains its minimum
by the hypothesis. Since , the function is strictly increasing and tends to infinity. There is consequently a unique first time satisfying
At a minimizer of , the numerator is nonzero because is nonzero, while the denominator tends to zero as . Hence the classical solution has gradient blow-up:
Under the inverse-flux quadratic bounds, smooth compactly supported data in a scalar conservation law satisfy
At the maximizing foot , the maximum representation for a concave conservation law bounds below by and above by . This bounds the deviation of the characteristic speed from ; the linear inverse-flux bound then controls . The time interval ends at the first characteristic crossing.