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Findthemomentum-spacewavefunctionϕn(p,t)forthenthstationarystateoftheinfinitesquarewell.Graph|ϕ1(p,t)|2and|ϕ2(p,t)|2,asfunctionsofp(payparticularattentiontothepointsp=±nπh/a).Useϕn(p,t)tocalculatetheexpectationvalueofp2.CompareyouranswertoProblem2.4.

Short Answer

Expert verified

The final result for the momentum-space time dependent wave function:ϕn(p,t)=πahne-iωntn2π2-a2p2/h2(1-(-1)neipa/h).

The expectation value ofp2=nπha2.

Step by step solution

01

Fourier transform  

A Fourier transform (FT) is a mathematical transformation that breaks down geographically or temporally dependent functions into spatially or temporally independent functions. First observe thenthin the coordinate representation for the infinite square well of width a: localid="1656312964496" ψn(x)=2asin(nπxa).

Now, the time-dependent solution to the given problem is just the stationary state multiplied by the time propagator:

localid="1656316815015" ψn(x,t)=2a-e-ntsin(nπxa).

Where the ωnis the abbreviation in the following context:

En=hωn=n2π2h22ma2

Now, the time dependent solution in the momentum representation is given by the Fourier transform of the coordinate basis, which connects the two basis. Therefore:

ϕn(p,t)=12πh-ψn(x,t)e-ipx/hdx=12πh2ae-iωnt0anπxae-ipx/hdx

The limits of the integration are from to since the wave function outside the box vanishes. Now isolate the integral and try to evaluate it.

l=0asin(Nx)e-kxdx

Where the abbreviations N=nπ/aand k=p/h.

02

Find the total solution to the integral l

Now rewrite the function in the terms of exponential function as follows:

sin(Nx)=12i(eiNx-e-iNx)

Therefore, the integrall has the following form:

l=0asin(Nx)e-ipx/hdx=0a12i(eiNx-e-iNx)e-ikxdx=12i0a(e-i(k-N)x-e-i(k+N)x)dx=l--l+

The integral lhas the following form:

l±=12i0ae-i(K±N)xdx=12ie-i(K±N)x-i(K±N)0a=12(K±N)(e-i(K±N)-1)

Therefore, the total solution to the integral lis:

l±=l--l+=12(K-N)(e-i(K-N)a-1)-12(K+N)(e-i(K+N)a-1)=e-i(Ka-nπ)2(K-N)-e-i(Ka+nπ)2(K+N)=(-1)ne-iKa2(K-nπ/a)-(-1)ne-iKa2(K+nπ/a)

03

Find momentum-space representation with the special case when n = 1 .

Now, combine this result for the integral with the time propagator and pre-factors, just obtain (by the use of common denominator) the final result for the momentum-space time dependent wave function: Φn(p,t)=πane-iωntn2π2-a2p2/2(1-(-1)ne-ipa/h)

Next, now that a general momentum-space representation is there find the special cases when n = 1 and n = 2 .

For n = 1 :

ϕ1(p,t)=πahe-iE1t/hπ2-a2p2/h2(1+e-ipa/h)=πahe-iE1t/hπ2-a2p2/h2e-ipa/2h(eipa/2h-e-ipa/2h)=2πahe-iE1t/hπ2-a2p2/h2e-ipa/2hcospa2h

Therefore, the square modulus can be simply obtained, a pure imaginary exponential function in the numerator is obtained:

ϕ2p,t2=4πahcos2(pa/2h(π2-a2p2/h2)2

04

Obtain the result for n = 2 and plot graph.

To obtain the result for n = 2, proceed in the similar manner as before, the only difference would now be that the factor (-1)nwill now yield a positive result, which in total will give a sin function. Since the steps are similar, they shall be skipped, so the final result is:

ϕ2(p,t)2=16πahsin2(pa/2h)(4π2-p2a2/h2)2

And the graph for the latter function has been shown below:

05

Find the expectation value of the  p2operator

To find the expectation value of the p2operator, first investigate how the momentum-space wave function depends on the parity of the number n. In the example for n = 1 and n = 2 the result obtained is sine and cosine functions. These numbers are by no means special; the same argument would hold for any other odd or even number n . Therefore, depending on the parity of the number n results can be obtained as sine or cosine function, as seen above. Next, it is important to notice that in momentum space, the expectation value of the p2operator is simply:

p2=-p2ϕ(p)2dp

Which in our case is simply by the use of the above facts about the parity of nfor the equation (1):

p2=4n2πah-p2(n2π2-a2p2/h2)2.Trig2(pa/2h)dp

Where the trig function is equal to cosine if n is odd and to sine if is even. The latter integral is not easy to evaluate, but it can be evaluated by a few different methods. One of the possibilities is to use complex analysis and evaluate the contour integral, second being partial fractions. Evaluate it for simplicity by the use of mathematics, since this is purely a mathematical step which brings no new important physics to the table. The integral, as some might've expected yields the same answer for either sine or cosine. The value of the integral is:

p2=nπha2

This is in agreement with the result of the problem 2.4 .

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Most popular questions from this chapter

Show that the energy-time uncertainty principle reduces to the "your name" uncertainty principle (Problem 3.14), when the observable in question is x.

Consider a three-dimensional vector space spanned by an Orthonormal basis 1>,2>,3>. Kets α>and β>are given by

|α=i|1-2|2-i|3,|β>=i|1+2|3.

(a)Construct<αand <β(in terms of the dual basis

1|,2|,3|).
(b) Find αβandβα,and confirm that

βα=αβ*.
(c)Find all nine matrix elements of the operatorA|αβ|, in this basis, and construct the matrix A. Is it hermitian?

The Hermitian conjugate (or adjoint) of an operator Q^is the operatorQ^such that

fQ^g=Q^fg (forallfandg).

(A Hermitian operator, then, is equal to its Hermitian conjugate:Q^=Q^)

(a)Find the Hermitian conjugates of x, i, andd/dx.

(b) Construct the Hermitian conjugate of the harmonic oscillator raising operator,a+(Equation 2.47).

(c) Show that(Q^R^)=R^Q^.

Suppose Ψ(x,0)=Ax2+a2.(-<x<)for constantsA and a.

(a) Determine A, by normalizingΨ(x,0)

(b) Find, and(at time).

(c) Find the momentum space wave functionΦ(p,0), and check that it is normalized.

(d) UseΦ(p,0)to calculatep,p2, andσp(at timet=0).

(e) Check the Heisenberg uncertainty principle for this state.

Show that two noncommuting operators cannot have a complete set of common eigenfunctions. Hint: Show that if P^and Q^have a complete set of common eigenfunctions, then [P^.Q^]f=0for any function in Hilbert space.

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