Show that

Ψ(x,t)=(mωπh)1/4exp[-mω2hx2+a221+e-2iωt+ihtm-2axe-iωt]

satisfies the time-dependent Schrödinger equation for the harmonic oscillator potential (Equation 2.43). Here a is any real constant with the dimensions of length. 46

(b) Find|Ψ(x,t)|2 and describe the motion of the wave packet.

(c) Compute <x> and <p> and check that Ehrenfest's theorem (Equation 1.38) is satisfied.

Short Answer

Expert verified

(a)The equation Ψ(x,t)=(πh)1/4exp[-2h(x2+a221+e-2iωt+ihtm-2axe-iωt)]conforms with the Schrödinger equation.

(b) The value of|Ψ|2ismωπhexp-mωhx-acosωt2.

(c) Ehrenfest's theorem is satisfied. <x>=acosωtand <p>=-maωsinωt.

Step by step solution

01

Define Ehrenfest's theorem

The Ehrenfest theorem is a specific example of a more general relationship between the expectation of any quantum mechanical operator and the expectation of the commutator of that operator with the Hamiltonian of the system, where A is the expectation value of some quantum mechanical operator.

dAdt=1ihH^,A^+A^t

02

Show that the equation satisfies the time-dependent Schrödinger equation

(a)

Here is an illustration of a precise solution to the harmonic oscillator potential part of the time-dependent Schrodinger equation:

Ψ(x,t)=(πh)1/4exp[-2h(x2+a221+e-2iωt+ihtm-2axe-iωt)]

Where a is a constant.

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

Ψt=-12ma2ω2e-2iωt+12hω+maxω2e-iωtΨ

The first derivative w.r.t x is:

Ψx=-mω2h2x-2ae-iωtψ=-mωhx-ae-iωtΨ

Also, the second derivative w.r.t x is:

2Ψx=-mωhΨx-ae-iωtΨx=-mωh+mωh2x-ae-iωt2Ψ

Assume,[s]=-h2m2x2+122x2Ψ

Thus:

[s]=-h2m-mωh+mωh2x-ae-iωt2Ψ+12mω2x2Ψ=12hω-12mω2x-2axeiωt2+12mω2x2Ψ=12hω+maxω2e-iωt-12mω2a2e-iωtΨ=ihΨt

Thus, the LHS and the So, LHS and RHS, of the Schrodinger equation are the same, that is:

-h22m2Ψx2+122x2Ψ=ihΨt

03

Explain the motion of the wave packet

(b)

Calculate the modulus square of the wave function,

ψ2=mωπhexp-mω2hx2+a221+e2iωt-ihtm-2axeiωt×expx2+a221+e2iωt+-ihtm-2axeiωtψ2=mωπhexp-mω2h2x2+a2+a2cos2ωt-4axcosωt

but:

a21+cos2ωt=2a2cos2ωt

So,

ψ2=mωπhexp-mωhx2-2axcosωt+a2cos2ωtψ2=mωπhexp-mωhx-acosωt2

Therefore, the wave packet center has a sinusoidal shape cosωt , and also it has a fixed Gaussian shape. The oscillations have an amplitude of a and an angular frequency of ω.

04

Find the expected momentum.

(c)

The expectation value of x is:

x=x|Ψ|2dx

let y = x -a cos ωtand thus dx = dy,

Now substitute

x=y+acosωt|Ψ|2dy

Now substitute from part (b) with and make the substitution with y,

So,

x=mωπh-y+acosωtexp-mωhy2dy

So we have two integrals, the first of which is zero, and the function is an odd function, as well as an odd function integration. -to is zero. To find the second integral, we use:

-e-bydy=πb

Therefore,

x=mωπhacosωtπhmω=acosωtx=acosωt

Hence, the value ofxis a cosωt.

The expectation value of the momentum is:

p=mdxdt=-maωsinωtp=-maωsinωt

Thus, the value of pis -maωsinωt.

Now check if the theorem is satisfied.

Here,

-dVdx=dpdtdpdt=-maω2cosωtV=12mω2x2dVdx=mω2x

-dVdx=-mω2x=-mω2acosωt=dpdt

Hence we conclude that Ehrenfest's theorem is satisfied.

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Most popular questions from this chapter

a) Show that the wave function of a particle in the infinite square well returns to its original form after a quantum revival time T = 4ma2/π~. That is: Ψ (x, T) = Ψ (x, 0) for any state (not just a stationary state).


(b) What is the classical revival time, for a particle of energy E bouncing back and forth between the walls?


(c) For what energy are the two revival times equal?

If two (or more) distinct44solutions to the (time-independent) Schrödinger equation have the same energy E . These states are said to be degenerate. For example, the free particle states are doubly degenerate-one solution representing motion to the right. And the other motion to the left. But we have never encountered normalizable degenerate solutions, and this is no accident. Prove the following theorem: In one dimension45 there are no degenerate bound states. Hint: Suppose there are two solutions, ψ1and ψ2with the same energy E. Multiply the Schrödinger equation for ψ1by ψ2and the Schrödinger equation for ψ2by ψ1and subtract, to show that ψ2dψ1/dx-ψ2dψ1/dxis a constant. Use the fact that for normalizable solutions ψ0at±to demonstrate that this constant is in fact zero.Conclude that ψ2s a multiple of ψ1and hence that the two solutions are not distinct.

Delta functions live under integral signs, and two expressions (D1xandD2x)involving delta functions are said to be equal if

-+f(x)D1(x)dx=-+f(x)D2(x)dxfor every (ordinary) function f(x).

(a) Show that

δ(cx)=1|c|δ(x)(2.145)

where c is a real constant. (Be sure to check the case where c is negative.)

(b) Let θ(x) be the step function:

θ(x){1,x>00,x>0(2.146).

(In the rare case where it actually matters, we define θ(0) to be 1/2.) Show that dθldx=δ

Analyze the odd bound state wave functions for the finite square well. Derive the transcendental equation for the allowed energies and solve it graphically. Examine the two limiting cases. Is there always an odd bound state?

A particle of mass m and kinetic energy E > 0 approaches an abrupt potential drop V0 (Figure 2.19).

(a)What is the probability that it will “reflect” back, if E = V0/3? Hint: This is just like problem 2.34, except that the step now goes down, instead of up.

(b) I drew the figure so as to make you think of a car approaching a cliff, but obviously the probability of “bouncing back” from the edge of a cliff is far smaller than what you got in (a)—unless you’re Bugs Bunny. Explain why this potential does not correctly represent a cliff. Hint: In Figure 2.20 the potential energy of the car drops discontinuously to −V0, as it passes x = 0; would this be true for a falling car?

(c) When a free neutron enters a nucleus, it experiences a sudden drop in potential energy, from V = 0 outside to around −12 MeV (million electron volts) inside. Suppose a neutron, emitted with kinetic energy 4 MeV by a fission event, strikes such a nucleus. What is the probability it will be absorbed, thereby initiating another fission? Hint: You calculated the probability of reflection in part (a); use T = 1 − R to get the probability of transmission through the surface.

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