A previous thread discusses the solution of the time-dependent Schrödinger equation for a massive particle in one dimension that starts off in the state Ψ(x,0)=δ(x). This can easily be solved in the momentum representation, giving the solution as Ψ(x,t)=12πeim2ℏtx2∫∞−∞e−iℏt2m(k−mℏtx)2dk,
Now, this procedure can sometimes seem a bit back-handed, and it leaves a lingering doubt of whether the solution in (∗) actually satisfies the differential equation iℏ∂∂tΨ(x,t)=−ℏ22m∂2∂x2Ψ(x,t)
While it might seem to be just a case of filling in the gaps, as a function of time, Ψ(x,t) is highly irregular at t=0, since it contains a singularity in the factor of e−isgn(t)π/4/√|t|=1/√it, and the exponential exp(imx22ℏt)=cos(mx22ℏ1t)+isin(mx22ℏ1t)
So, just to fill in the gaps: in what sense, and without referring to the momentum representation, is (∗) a solution of (S)?
Answer
Sketched proof: If we define a regularized distribution
Ψϵ[f;t] := ∬R2dx dk2π f(x)exp{ikx−ℏk22m(ϵ+it)} = √m2πℏ(ϵ+it)∫Rdx f(x)exp{−mx22ℏ(ϵ+it)},t ∈ R,ϵ ∈ R+,
for a spatial test function f, one may show firstly via Lebesgue's dominated convergence theorem that Ψϵ[f;t] becomes the Dirac delta distribution
limϵ→0+limt→0Ψϵ[f;t] = δ[f] := f(0)fort → 0,
and secondly that the regularized Ψϵ[f;t] satisfies TDSE for t∈R and ϵ∈R+. Here the spatial derivative Ψϵ,xx[f;t] := Ψϵ[fxx;t]
No comments:
Post a Comment