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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.

Short Answer

Expert verified

a) The value of A=2a3π

b) The value are as followsσx=a, x2=a2,and x=0

c) The momentum space wave function is ae-|p|a/

d) The value are as follows p=0, p2=22a2,andσp=2a

e) After finding the expectation values one can obtain the uncertainties for acquainted observables.

Step by step solution

01

Determine A , by normalizing Ψ(x,0)

a)

It is easy to obtain the constant A by requiring wave function to be normalized, more formally as:

-|ψ(x)|2dx=1

Which in this case turns into the following requirement:

-A2x2+a22dx=1

Integrate using Mathematica but the integral can be calculated by the use of reduction formula to reduce the integral into several integrals with lower power in the denominator. The integral turns out to be:

-A2x2+a22dx=12A2a3π12A2a3π=1A=2a3π

Thus, the value of A is2a3π

02

Find  ⟨x⟩,x2, and  σx(at time t=0  ).

b)

Let us calculate the required expectation values:

x=-x·A2x2+a22dx=0

The integral is trivially zero, because of integrating an odd function on a symmetric interval. The next expectation value can be obtained as follows:

x2=-x2·A2x2+a22dx

Again, this is not a simple integral, but can be analysed analytically by writing x2=x2+a2-a2to obtain two integrals:

-A2x2x2+a22=A2-x2+a2-a2x2+a22=A2-x2+a2x2+a22dx--a2x2+a22dx=A2-1x2+a2dx--a2x2+a22dx

The last two integrals are trivial, since the first one is a table integral and the second one was calculated in the previous part of the problem where the question asked to find the normalization constant. Therefore, the integrals are trivial and yield the following value:

x2=A2π2a=2a3ππ2a=a2

Now, calculate the uncertainty, σx. It is defined as follows:

σx=x2-x2=a2-0σx=a

Thus, the value ofx,x2, andσx are 0, a2,andarespectively.

03

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

c)

To find the momentum space wave function,find the Fourier transform of the original coordinate space wave function, since it is a connection between these two different representations. Therefore:Φ(p)=12π-ψ(x)e-ipx/dx

In this case this becomes the following:

Φ(p)=12π-Ax2+a2e-ipx/dx=12π-Ax2+a2[cos(px/)-isin(px/)]dx

In the last stepuse the trigonometric expression for the exponential function. Now, the last integral separates into two integrals; one with sine and second with cosine function. The sine integral vanishes, because of integrating an odd function on a symmetric interval. Therefore, only need focus on the cosine integral:
Φ(p)=12π-Acos(px/)x2+a2dx=2A2ππ2ae-|p|a/Φ(p)=ae-|p|a/

Now, to check whether this function is normalized, weintegrate over all momentum space as follows:

-|Φ(p)|2dp=-ae-2|p|a/dp=2·0ae-2pa/dp=1

In the last step use several properties, one being that the wave function is even and therefore integrate from to and multiply it by two, instead of integrating over the whole space. Integrate only in the positive domain of P , the absolute value in the exponential function turns out to be |p|=p, and the latter integral is then trivial.

04

Use Φ(p,0) to calculate⟨p⟩,p2 , and  σp(at time t = 0  ). 

d)

To find the desired expectation values, we can either work in the coordinate or momentum space. Since we already have the momentum space wave function, it is simpler to work in it (since the expectation values are just integrals of the wave function multiplied by the momentum P , same as expectation value of position in the coordinate space calculations). Then:

p=-pΦ(p)dp=-pae-2|p|a/dp=0

This integral is again equal to 0, since we are integrating an odd function on a symmetric interval. Next, we need to find the expectation value of the squared momentum operator

p2=-p2Φ(p)dp=-p2ae-2|p|a/dp=20p2ae-2pa/dp

Now, this integral can evaluated by integrating by parts twice. This is messy and takes time and there is no physics behind it, so I shall again evaluate the integral using Mathematica. If someone wishes to do it by hand, I have written the procedure required to do it. The expectation value turns out to be:

σp=p2-p2=22a2-0σp=2a

Therefore, the uncertainty is given by:

Thus, the value of , p, localid="1659011703261" p2and σpare 0, localid="1659011735931" 22a2,and rlocalid="1659011745980" 2aespectively.

05

Check the Heisenberg uncertainty principle for this state.

e)

To check whether the uncertainty relation holds, we need to multiply the two uncertainties as follows:σxσp=a2a=2=2·2>2

Therefore, the uncertainty relation is satisfied.

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Most popular questions from this chapter

(a) Show that the set of all square-integrable functions is a vector space (refer to Section A.1 for the definition). Hint: The main problem is to show that the sum of two square-integrable functions is itself square-integrable. Use Equation 3.7. Is the set of all normalized functions a vector space?

(b) Show that the integral in Equation 3.6satisfies the conditions for an inner product (Section A.2).

In an interesting version of the energy-time uncertainty principle31, t=τ/πwhere τis the time it takesΨ(x,t)to evolve into a state orthogonal toΨ(x,0) . Test this out, using a wave function that is an equal admixture of two (orthonormal) stationary states of some (arbitrary) potential:Ψ(x,0)=(1/2)[Ψ1x+Ψ2(x)]

Test the energy-time uncertainty principle for the free particle wave packet in Problem 2.43and the observable x , by calculating σHσx , and d<x>/dtexactly.

Show that if hQ^h=Q^hhfor all functionsh(in Hilbert space), thenfQ^g=Q^fgfor allrole="math" localid="1655395250670" fandg(i.e., the two definitions of "Hermitian" -Equations 3.16 and 3.17- are equivalent).

Coherent states of the harmonic oscillator. Among the stationary states of the harmonic oscillator (Equation 2.67) only n = 0 hits the uncertainty limit (σxσp=h/2); in general, σxσp=(2n+1)h/2, as you found in Problem 2.12. But certain linear combinations (known as coherent states) also minimize the uncertainty product. They are (as it turns out) Eigen functions of the lowering operator

ψn=1n!(a^+)nψ0(2.68).

a_|α>=α|a>(the Eigen value α can be any complex number).

(a)Calculate <x>,<x2>,<p>,<p2>in the state |α〉. Hint: Use the technique in Example 2.5, and remember that is the Hermitian conjugate of a-. Do not assume α is real.

(b) Find σx; show that σxσp=h/2.

(c) Like any other wave function, a coherent state can be expanded in terms of energy Eigen states: |α>=n=0Cn|n>.

Show that the expansion coefficients arecn=αnn!c0.

(d) Determine by normalizing |α〉. Answer: exp(-α2/2)

(e) Now put in the time dependence: |n>e-iEntIh|n>,

and show that |αt|remains an Eigen state of a-, but the Eigen value evolves in time:α(t)=e-iωt So a coherent state stays coherent, and continues to minimize the uncertainty product.

(f) Is the ground state (n=0>)itself a coherent state? If so, what is the Eigen value?

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