Consider the moving delta-function well: V(x,t)=-αδ(x-vt)

where v is the (constant) velocity of the well. (a) Show that the time-dependent Schrödinger equation admits the exact solution ψ(x,t)=he-|x-vt|lh2e-i[E+1/2mv2t-mvx]lhwhere E=-2l2h2 is the bound-state energy of the stationary delta function. Hint: Plug it in and check it! Use the result of Problem 2.24(b). (b) Find the expectation value of the Hamiltonian in this state, and comment on the result.

Short Answer

Expert verified

(a)The time-dependent Schrödinger equation conforms with the exact solution.

(b) The expectation value of the Hamiltonian in this state is H=E+12mv2.

Step by step solution

01

Define Hamiltonian

When time is not explicitly included in the function, it is equal to the total energy of the system. It is used to describe a dynamic system (such as the motion of a particle) in terms of components of momentum and coordinates of space and time, and it is equal to the total energy of the system.

02

Establish the equation to be true

(a)

An exact solution to the time-dependent Schrodinger equation with the moving delta-function wellVx,t=-αδx-vt, is given by:

ψx,t=mαhe-mαx-vtlh2e-iE+mv2l2t-mvxlh

Prove that this wave function satisfies the Schrodinger equation. The first derivative w.r.t is:

ψt=-mαh2v2θx-vt-1-iE+12mv2hψThus:ihψt=imαvh22θx-vt-1+E+12mv2ψ

Where:

tx-vt=-Vifx-vt>0V,ifx-vt<0

the function θis defined by equation 2.143 as:

θx=1x<00x>0

Using this definition, we can write equation (2) as:

tx-vt=-v2θx-vt-1

Substitute with this equation into (1) to get:

ψt=mαh2v2θx-vt-1-iE+12mv2hψ

Thus;

ihψt=imαvh2θx-vt-1+E+12mv2ψ

The first derivative w.r.t x is;

2ψx2=-mαh22θx-vt-1+imvh2ψ-2mαhxθx-vtψ

Note that,

xθx-vt=δx-vt

Thus,

-h22m2ψx2=-h22m-mαh22θx-vt-1+imvh2ψ+αδx-vtψ=-h22m-mαh22θx-vt-1+imvh2ψ+αδx-vtψ=-h22m-m2α2h42θx-vt-12-m2v2h2=-2imvhmαh2θx-vt-1+αδx-vtψ

Now 2θx-vt-12=1,thus:-h22m2ψx2=-mα22h2+12mv2+imvαh2θx-vt-1+αδx-vtψ-h22m2ψx2-αδx-vtψ=-mα22h2+12mv2+imvαh2θx-vt-1ψ

Also,E=12mv2,thus:-h22m2ψx2-αδx-vtψ=ihψt

Therefore, the time-dependent Schrödinger equation conforms with the exact solution.

03

Find the expectation value of the Hamiltonian,

(b)

The expectation value of Hamiltonian is expressed by the equation,

H=-ψ*Hψdx

Here,

Hψ=ihψt

which is determined in part (a) and substituted into the following equation in equation (3); we get:

role="math" localid="1658299633201" H-mαvh2θx-vt-1+E+12mv2ψ*ψ

Let y=x-vt

thus:

H-mαvh2θx-vt-1+E+12mv2ψ2

from the normalization -ψ2=1and 2θx-vt-1 is an odd function, and the integration of an odd function from - to is zero,

so:

H=E+12mv2

Thus, the expectation value of the Hamiltonian in this state isH=E+12mv2 .

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Most popular questions from this chapter

A particle of mass m is in the ground state of the infinite square well (Evaluation 2.19). Suddenly the well expands to twice its original size – the right wall moving from a to 2a – leaving the wave function (momentarily) undisturbed. The energy of the particle is now measured.

  1. What is the most probable result? What is the probability of getting that result?
  2. What is the next most probable result, and what is its probability?
  3. What is the expectation value of the energy? (Hint: if you find yourself confronted with an infinite series, try another method)

Show that there is no acceptable solution to the Schrodinger equation for the infinite square well with E=0orE<0(This is a special case of the general theorem in Problem 2.2, but this time do it by explicitly solving the Schrodinger equation, and showing that you cannot meet the boundary conditions.)

The scattering matrix. The theory of scattering generalizes in a pretty obvious way to arbitrary localized potentials to the left (Region I),V(x)=0soψ(x)=Aeikx+Be-ikx,wherek2mE

To the right (Region III),V(x)is again zero, soψ(x)=Feikx+Ge-ikxIn between (Region II), of course, I can't tell you what is until you specify the potential, but because the Schrödinger equation is a linear, second-order differential equation, the general solution has got to be of the form

ψwhere f(x)and g(x)are two linearly independent particular solutions. 48 There will be four boundary conditions (two joining Regions I and II, and two joining Regions II and III). Two of these can be used to eliminate C and D, and the other two can be "solved" for B and F in terms of \(A\) and G

B=S11A+S12G.F=S21A+S22G

The four coefficientsSijwhich depend on k (and hence on E), constitute a2×2matrix s called the scattering matrix (or S-matrix, for short). The S-matrix tells you the outgoing amplitudes (B and F) in terms of the incoming amplitudes (A and G):

(BF)=(S11S21S21S22)(AG)

In the typical case of scattering from the left, G=0so the reflection and transmission coefficients are

Rl=|B|2|A|2|G=0=|S11|2.TI=|F|2|A|2|G=0=|S2|2.

For scattering from the right, and

Rr=|F|2|G|2A=0=|S22|2.Tr=|B|2|G|2A=0=|S12|2.

(a) Construct the S-matrix for scattering from a delta-function well (Equation 2.114). (b) Construct the S-matrix for the finite square well (Equation 2.145). Hint: This requires no new work, if you carefully exploit the symmetry of the problem.

A particle of mass m in the infinite square well (of width a) starts out in the left half of the well, and is (at t=0) equally likely to be found at any point in that region

(a) What is its initial wave function, ψ(x,0)? (Assume it is real. Don’t forget to normalize it.)

(b) What is the probability that a measurement of the energy would yield the valuesπ2h22ma2?

Evaluate the following integrals:

(a)-3+1(x3-3x2+2x-1)δ(x+2)dx.

(b).0[cos(3x)+2]δ(x-π)dx

(c)_1+1exp(lxl+3)δ(x-2)dx

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