Alphabeta Math
DefinitionDefinition: Literature-sourcedProof: Not applicablePipeline-generatedjudge pass (gpt-6.1-sol)
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Wave equation, Cauchy data and wave speed

Definition

Let n≥1, T>0 and c>0, let ∂t,∂j be the partial derivatives of Directional derivatives and partial derivatives of a map U⊆Rm→Rn and let Δ=∑j=1n∂j2 be the Laplacian of The Laplacian of a C2 function and of a C2 vector field. The wave operator of speed c is □c:=∂t2−c2Δ, and the wave equation with source f is the equation □cu=f on a slab Rn×(0,T); the equation is homogeneous when f=0. A classical solution on the time slab Rn×[0,T) is a function u of class C2 on Rn×(0,T) in the sense of Ck maps and multi-index derivative notation in Euclidean space which satisfies the equation at every point of Rn×(0,T). This is the classical-solution and Cauchy-data vocabulary of Scalar partial differential equations, order, and classical solutions, and □c is a linear second-order operator in the sense of Linear, semilinear, quasilinear, and fully nonlinear partial differential equations.

The Cauchy problem for □cu=f prescribes a displacement u0:Rn→R and a velocity u1:Rn→R and asks for a classical solution attaining them as t↓0 in the pointwise sense: u(x,t)→u0(x) and ∂tu(x,t)→u1(x) for every x∈Rn as t↓0. Only the limits are part of the data, so u need not be defined at t=0 a priori.

Unit-speed rescaling convention. A function u solves □cu=0 on Rn×[0,T) with data (u0,u1) if and only if v(x,s):=u(x,s/c) solves ∂s2v=Δv on Rn×[0,cT) with data (u0,u1/c); equivalently u(x,t)=v(x,ct). Indeed continuous coordinate partial derivatives imply total differentiability (If all partial derivatives exist on a neighbourhood and are continuous at a point, then the map is totally differentiable there with Jacobian derivative), so the chain rule (The chain rule for total derivatives: D(g∘f)(a)=Dg(f(a))∘Df(a)) gives ∂tu(x,t)=c ∂sv(x,ct) and ∂t2u(x,t)=c2∂s2v(x,ct) while spatial derivatives are unchanged, so □cu=c2(∂s2v−Δv) evaluated at s=ct, and the initial displacement limits agree, while the initial velocity limit of u is c times that of v. The cited treatments state their formulas at unit speed, and this convention is the only place where the general speed enters those formulas.

Sphere normalisation. Let σ be the polar surface measure on the unit sphere (The polar surface set function on the unit sphere). Write Vm:=∣B1m∣ for the unit ball and ωm:=σ(Sm)=(m+1)Vm+1>0 for the total polar measure of the unit sphere Sm⊆Rm+1 (Sphere and ball measures scale in Rn); thus the boundary sphere of a ball in Rn has total measure ωn−1=nVn. For an integer m≥0 put (2m+1)!!:=(2m+1)(2m−1)⋯3⋅1 and (2m)!!:=(2m)(2m−2)⋯2, so that 0!!=1!!=1 and (n−2)!! is defined for every odd n≥3. All sphere and weighted-ball integrals on this page are read under the Axiom of Countable Choice of The Axiom of Countable Choice (ACω), under which the polar measure and its integrals are supplied.

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