Question:

An illuminating alternative derivation of the WKB formula (Equation) is based on an expansion in powers ofh. Motivated by the free particle wave function ψ=Aexp(±ipx/h),, we write

ψ(x)=eif(x)/h

Wheref(x)is some complex function. (Note that there is no loss of generality here-any nonzero function can be written in this way.)

(a) Put this into Schrödinger's equation (in the form of Equation8.1), and show that

. ihfcc-(fc)2+p2+0.

(b) Write f(x)as a power series inh:

f(x)=f0(x)+hf1(x)+h2f2(x)+......And, collecting like powers ofh, show that

(o˙0)2=p2,io˙0=2o˙0o˙1,io˙1=2o˙0o˙2+(o˙1)2,....

(c) Solve forf0(x)andf1(x), and show that-to first order inyou recover Equation8.10.

Short Answer

Expert verified

(a)ihf"-(f')2+p2=0 And it’s proved.

(b)(f0')2=p2,if0:=2f0'f1',if1:=2f0'f2'+(f1')2 and it’s proved.

(c)Therefore, ψ(x) is given by

ψ(x)cp(x)e±ihp(x)dx

Step by step solution

01

Step 1:(a) Show the Schrodinger Equation.

Let, the wave equation take the form,

ψ(x)=eif(x)/h

Where, f(x) is some complex function.

So that,

dψdx=ihf'(x)ψ(x)d2ψdx2=ihf"(x)-1h2f'(x)2ψ(x)...(a)

We known that Schrodinger Equation,

d2ψdx2=p2h2ψ

Substitute equation (a) in Schrodinger Equation we get,

if"h-f'2h2ψ(x)=-p2h2ψ(x)This leads to

ihf"-f'2+p2=0 ............(1)

02

(b) To write f(x) as a power series.

Writeas a power series in:

f(x)=f0(x)+hf1(x)+h2f2(x)+...,

So that,

f'(x)=f0'x)+hf1'(x)+h2f2'(x)+...,f"(x)=f0"x)+hf1"(x)+h2f2"(x)+...,

Putting this into equation (1) we have,

ihf0"+hf1"+h2f2"+...,-f0'+hf1'+h2f2'+...,+p2=0

(Or)

p2-f0'2+hif0"-2f0'f1'+h2if0"-2f0'f2'-f1'2+Oh3

Finally, power of yields,

f0'2=p2,if0"-2f0'f1',if0"-2f0'f2'-f1'2

........etc.

03

Step 3:(c) To solve f0(x) and f1(x).

In step 2, we have to show that,

f0'2=p2

(or)

f0'=±p

Integrating we get,

f0x=±pxdx+C1(C1 is constant)

Also, it follows (by taking the x-derivative) that,

f0"=±dpdx

Again from step 2, we have shown that

if0"=2f0'f1'

Solving for f1'an substituting for f0'and f0'then,

f1'=i2pdpdx=i2dinpxdx

By integrating, we get

f1'=i2inpx+C2(C2 is constant)

Hence, we can write f(x) into first order in has,

role="math" localid="1658465427689" fx=±pxdx+ihInp(x)+constant+Oh2

Hence ψ(x)is given by,

ψ(x)exp±ihpxdx-ihInp(x)+constant=Cp(x)e±ihpxdx

Which is exactly as equation (8.10).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

About how long would it take for a (full) can of beer at room temperature to topple over spontaneously, as a result of quantum tunneling? Hint: Treat it as a uniform cylinder of mass m, radius R, and height h. As the can tips, let x be the height of the center above its equilibrium position (h/2) .The potential energy is mgx, and it topples when x reaches the critical value X0=R2+(h/2)2-h/2. Calculate the tunneling probability (Equation
8.22), for E = 0. Use Equation 8.28, with the thermal energy ((1/2)mv2=(1/2)kBT)to estimate the velocity. Put in reasonable numbers, and give your final answer in years.

Te-2T,withγ1h0a|px|dx... (8.22).

tau=2r1Ve2T (8.28).

Calculate the lifetimes of U238andPo212, using Equations8.25and 8.28 . Hint: The density of nuclear matter is relatively constant (i.e., the same for all nuclei), sor13is proportional to (the number of neutrons plus protons). Empirically,

r1=(1.07fm)A1/3

Consider the quantum mechanical analog to the classical problem of a ball (mass m) bouncing elastically on the floor.
(a) What is the potential energy, as a function of height x above the floor? (For negative x, the potential is infinite x - the ball can't get there at all.)
(b) Solve the Schrödinger equation for this potential, expressing your answer in terms of the appropriate Airy function (note that Bi(z) blows up for large z, and must therefore be rejected). Don’t bother to normalize ψ(x).
(c) Using g=9.80m/s2and m=0.100kg , find the first four allowed energies, in joules, correct to three significant digits. Hint: See Milton Abramowitz and Irene A. Stegun, Handbook of Mathematical Functions, Dover, New York (1970), page 478; the notation is defined on page 450.
(d) What is the ground state energy, in ,eV of an electron in this gravitational field? How high off the ground is this electron, on the average? Hint: Use the virial theorem to determine <x> .

Consider the case of a symmetrical double well, such as the one pictured in Figure. We are interested in Figure 8.13bound states with E<V(0) .
(a) Write down the WKB wave functions in regions (i) x>x2 , (ii) x1<x<x2 , and (iii) 0<x<x1. Impose the appropriate connection formulas at and (this has already been done, in Equation 8.46, for x2 ; you will have to work out x1 for yourself), to show that


ψ(x)={DPxexp-1hx2xpx'dx'2DPxsin1hx2xpx'dx'+π4DPx2cosθ1hvx1pxdx+sinθe1hvx1pxdx

FIGURE 8.13: Symmetrical double well; Problem 8.15.
Where

θ1hx1x2p(x)dx .

(b) Because v(x) is symmetric, we need only consider even (+)and odd (-)wave functions. In the former case ψ(0)=0 , and in the latter case ψ=(0)=0 . Show that this leads to the following quantization condition:

tanθ=±2ef.

Where

f1h-x1x1p(x)dx

Equation 8.59determines the (approximate) allowed energies (note that Ecomes into 1 and x2, so θ and ϕ are both functions of E ).

(c) We are particularly interested in a high and/or broad central barrier, in which case ϕ is large, and eϕis huge. Equation 8.59 then tells us thatA θmust be very close to a half-integer multiple of π . With this in mind, write localid="1658823154085" (θ=n+1/2)π+o . where localid="1658823172105" ||<<1, and show that the quantization condition becomes

localid="1658823190448" θ=(n+12)πm12e-f.

(d) Suppose each well is a parabola: 16

localid="1658823244259" v(x)={12mω2x+a2,ifx<012mω2x-a2,ifx<0 .

Sketch this potential, find (Equation 8.58 ), and show that

localid="1658823297094" En±=(n+12)hωmhω2πe-f

Comment: If the central barrier were impenetrable localid="1658823318311" (f) , we would simply have two detached harmonic oscillators, and the energies, localid="1658823339386" En=(n+1/2)hω , would be doubly degenerate, since the particle could be in the left well or in the right one. When the barrier becomes finite (putting the two wells into "communication"), the degeneracy is lifted. The even (localid="1658823360600" ψn+) states have slightly lower energy, and the odd ones ψn. have slightly higher energy.
(e) Suppose the particle starts out in the right well-or, more precisely, in a state of the form

localid="1658823391675" ψ(x,0)=12(ψn++ψn)

which, assuming the phases are picked in the "natural" way, will be concentrated in the right well. Show that it oscillates back and forth between the wells, with a period

localid="1658823416179" τ=2π2ωe.

(f) Calculate , for the specific potential in part (d), and show that for , localid="1658823448873" V(0).>>E,ϕ~mωa2/h.

Use the WKB approximation to find the allowed energies of the general power-law potential:

V(x)=α|x|vwhere v is a positive number. Check your result for the case v=2 .

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free