A particle in the infinite square well (Equation 2.22) has the initial wave function Ψ (x, 0) = A sin3(πx/a) (0 ≤ x ≤ a). Determine A, find Ψ(x, t), and calculate 〈x〉as a function of time. What is the expectation value of the energy? Hint: sinnθ and cosnθ can be reduced, by repeated application of the
trigonometric sum formulas, to linear combinations of sin(mθ) and cos(mθ), with m = 0, 1, 2, . . ., n.

Short Answer

Expert verified

A=45aψ(x,t)=15a3exp-iπ2h2ma2tsinπxa-exp-i9π2h2ma2tsin3πxax=a2Expectationvalueforenergy,E=9π2h210ma2

Step by step solution

01

The Partial differential equation:

Schrodinger equation is given by,

ihψt=h22m2ψx2+V(x,t)ψ(x,t)

For an infinite square well,

V(x,t)=V(x)=0,0<x<a,otherwise

Reducing the partial differential equation to two ordinary differential equations in x and t:

ihϕ'(t)ϕ(t)=E-h22mψ''(x)ψ(x)=E

In the boundary conditionsψ(0)=0and ψ(a)=0, the time-independent Schrödinger equation gives normalized solutions of the form,

ψn(x)=2asinnπxaEn=n2π2h22ma2

Using this formula, the solution to the ordinary differential equation in t is ϕn(t)=e-iEnt/h. The general solution for ψ(x,t)is a linear combination of the product solutions ϕn(t)ψn(x)for all n.

02

General solution

By using the general solution

ψ(x,t)=n-1cnϕn(t)ψn(x)ψ(x,t)=n-1cn2aexp-in2π2h2ma2sinnπxa

at t = 0

ψ(x,0)=n-1cn2asinnπxaψ(x,0)=Asin3πxaψ(x,0)=Aeinx/a-e-inx/a2i3ψ(x,0)=Ae3inx/a-3e-inx/a+3e-inx/a-e-3inx/a8i3ψ(x,0)=A34einx/a-e-inx/a2i-14e3inx/a-e-3inx/a2iψ(x,0)=3A4sinπxa-A4sin3πxaψ(x,0)=3A4a2ψ1(x)-A4a2ψ3(x)


Comparing the coefficients,

c12a=3A4,n=1c12a=A4,n=3c12a=0,n1&n3

Hence,

localid="1658294538499" ψ(x,t)=3A4exp-iπ2h2ma2tsinπxa-A4exp-i9π2h2ma2tsin3πxa

03

Normalising the wave function

Here the wave function is:

1=0aψ(x,0)2dx1=0a3A4a2ψ1x-A4a2ψ3x2dx1=0a9A216a2ψ1x2-23A4A4a2ψ1(x)ψ3x+A216a2ψ3(x)2dx

Using the orthonormality of eigenstates to evaluate this integral,

1=5aA216A=45a

Hence, the wave function becomes,

ψ(x,t)=15a3exp-iπ2h2ma2tsinπxa-exp-i9π2h2ma2tsin3πxa

In terms of eigenstates,

ψ(x,t)=3A4a2ψ1(x)e-iE1t/h-A4a2ψ3(x)e-iE3t/hψ(x,t)=310ψ1(x)e-iE1t/h-110ψ3(x)e-iE3t/h

04

Calculating the expectation value of energy

The expectation value of energy can be calculated as:

E=ncn2EnE=c12E1+c32E3E=E13102+E3-1102E=910E1+110E3E=910×π2h22ma2+110×9π2h22ma2E=9π2h210ma2

05

Calculating the expectation value of x

The expectation value of x can be calculated here as:

x=0aψ*x,txψ(x,t)dxx=0ax15a3exp-iπ2h2ma2tsinπxa-exp-i9π2h2ma2tsin3πxadx15a3expiπ2h2ma2tsinπxa-expi9π2h2ma2tsin3πxax=15a0ax9sin2πxa+sin23πxa-6cos4π2hma2tsinπxasin3πxadx

Splitting up the integral and evaluating it, we get,

x=95a0axsin2πxadx+15a0axsin23πxadx-65acos4π2hma2t0axsinπxasin3πxadxx=a2-910π0-110π0-35πcos4π2hma2t0-0x=a2

Calculated values are :A=45a

role="math" localid="1658296781760" ψ(x,t)=15a3exp-iπ2h2ma2tsinπxa-exp-i9π2h2ma2tsin3πxax=a2

Expectation value for energy, E=9π2h210ma2

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Most popular questions from this chapter

This is a strictly qualitative problem-no calculations allowed! Consider the "double square well" potential (Figure 2.21). Suppose the depth V0and the width a are fixed, and large enough so that several bound states occur.

(a) Sketch the ground state wave function Ψ1and the first excited state localid="1658211858701" Ψ2(i) for the case b = 0 (ii) forbaand (iii) for ba

(b) Qualitatively, how do the corresponding energies(E1andE2)and vary, as b goes from 0 to ? Sketch E1(b)and E2(b)on the same graph.

(c) The double well is a very primitive one-dimensional model for the potential experienced by an electron in a diatomic molecule (the two wells represent the attractive force of the nuclei). If the nuclei are free to move, they will adopt the configuration of minimum energy. In view of your conclusions in (b), does the electron tend to draw the nuclei together, or push them apart? (Of course, there is also the internuclear repulsion to consider, but that's a separate problem.)

a) Compute x,p,x2,p2, for the states ψ0and ψ1, by explicit integration. Comment; In this and other problems involving the harmonic oscillator it simplifies matters if you introduce the variable ξmωxand the constant α(mωπ)1/4.

b) Check the uncertainty principle for these states.

c) Compute T(the average kinetic energy) and V(the average potential energy) for these states. (No new integration allowed). Is their sum what you would expect?

In this problem we explore some of the more useful theorems (stated without proof) involving Hermite polynomials.

a. The Rodrigues formula says thatHn(ξ)=(1)neξ2(d)neξ2

Use it to derive H3 and H4 .

b. The following recursion relation gives you Hn+1 in terms of the two preceding Hermite polynomials: Hn+1(ξ)=2ξHn(ξ)2nHn1(ξ)

Use it, together with your answer in (a), to obtain H5 and H6 .

(c) If you differentiate an nth-order polynomial, you get a polynomial of

Order (n-1). For the Hermite polynomials, in fact,

dHn=2nHn1(ξ)

Check this, by differentiatingH5and H6.

d. Hn(ξ)is the nth z-derivative, at z = 0, of the generating function exp(z2+2ξz)or, to put it another way, it is the coefficient ofznn! in the Taylor series expansion for this function: ez2+2ξz=n=0znn!Hn(ξ)

Use this to obtain H0,H1and H2.

The gaussian wave packet. A free particle has the initial wave function

Y(x,0)=Ae-ax2

whereAand are constants ( is real and positive).

(a) NormalizeY(x,0)

(b) Find Y(x,t). Hint: Integrals of the form

-+e-(ax2+bx)dx

Can be handled by “completing the square”: Lety=a[x+bl2a], and note that(ax2+bx)=y2-(b2l4a). Answer:

localid="1658297483210" Y(x,t)=(2aπ)1/4e-ex2l[1+(2ihatlm)]1+(2ihatlm)

(c) Find . Express your answer in terms of the quantity

localid="1658297497509" ω=a1+(2ihatlm)2

Sketchlocalid="1658124147567" |Y|2(as a function of x) at t=0, and again for some very large t. Qualitatively, what happens to |Y|2, as time goes on?

(d) Find <x>,<p>,<x2>,<p2>,σxand σP. Partial answer:localid="1658297458579" <p2>=ah2, but it may take some algebra to reduce it to this simple form.

(e) Does the uncertainty principle hold? At what time tdoes the system come

closest to the uncertainty limit?

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?

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