For spherically symmetrical potentials we can apply the WKB approximation to the radial part (Equation 4.37). In the case I=0it is reasonable 15to use Equation 8.47in the form

0r0p(r)dr=(n-1/4)πh.

Where r0is the turning point (in effect, we treat r=0as an infinite wall). Exploit this formula to estimate the allowed energies of a particle in the logarithmic potential.

V(r)=V0In(r/a)

(for constant V0and a). Treat only the case I=0. Show that the spacing between the levels is independent of mass

Short Answer

Expert verified

The radial part of the energy level E is,

En=V0In2πmV0n-14haEn+1-En=V0Inn+3/4n-1/4

Step by step solution

01

To determine the energy by using radial equation. 

The radial equation for hydrogen is given by:

-h22md2udr2+Vr+h22mII+1r2u=Eu

Where u(r) .The simplest case is when I=0, that is:

-h22md2udr2+Vru=Eu …………………..(1)

The WKB functions on either side of the turning point, for an increasing potential are given by:

ur=2Dprsinrr2prdr'/h+π/4r<r2Dprexp-r2rprdr'/hr>r2

Where r2is the turning point. But urmust be zero at r=0 , so the sine function must equal zero at this point, the sine function equals zero when the value inside it is equal to nπthat is:

0r2prdr/h+π4=0r2prdr=n-14πh.......................2

The potential that we want to apply the approximations on it is:

Vr=V0Inra ……………………….(3)

The turning point can be determined by setting the potential at this point equal to the energy that is:

E=V0Inr2aE=V0Inr2a …………………………….(4)

02

To find the integral value.

Now we need to find the integral in (2), where

pr=2mE-V

So we have:

0r2prdr=2m0r2E-V0Inradr0r2prdr=2m0r2V0Inra-V0Inradr

By using the following substitutions,

v=Inr2rdv=rr0-r0r2drv=-1rdrdv=-evr0dr

And also change the limits r=0u=andr=r2u=0we get:

0f2prdr=2mV00f2Inr2rdr0f2prdr=r22mV00ve-vdvΓ320f2prdr=2πmV0r22

Substitute into (2) we get:

n-14πh=2πmV0r22

03

To find spacing energy levels.

Solve for r2to get:

localid="1658383846287" r2=2πmV0n-14h …………………(5)

Solve equation (4) for r2, to get:

r2=aeE/V0

Substitute into (5) with r2, so we get:

aeE/V0=2πmV0n-14h

Solve for E to get:

En=V0In2πmV0n-14ha

The spacing between energy levels with n and n+1 is:

En+1-E=V0In2πmV0n+34ha-In2πmV0n-14ha

Using, (A) -In (B) =In(A/B) ,we get:

En+1-En=V0Inn+3/4n-1/4Which is independent of m and a.

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Most popular questions from this chapter

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.

As an explicit example of the method developed inProblem 7.15, consider an electron at rest in a uniform magnetic fieldB=B2Kfor which the Hamiltonian is (Equation 4.158):

H=-γB (4.158).

H0=eBzmSz (7.57).

The eigenspinors localid="1656062306189" xaandxbandthecorrespondingenergies,EaandEb, are given in Equation 4.161. Now we turn on a perturbation, in the form of a uniform field in the x direction:

{x+,withenergyE+=-γB0ħ/2x-,withenergyE-=-γB0ħ/2 (4.161).

H'=ebxmSx (7.58).

(a) Find the matrix elements of H′, and confirm that they have the structure of Equation 7.55. What is h?

(b) Using your result inProblem 7.15(b), find the new ground state energy, in second-order perturbation theory.

(c) Using your result inProblem 7.15(c), find the variation principle bound on the ground state energy.

Derive the connection formulas at a downward-sloping turning point, and confirm equation8.50.

ψ(x)={D'|p(x)|exp-1hxx1|p(x')|dx'.ifx<x12D'p(x)sin-1hx1xp(x')dx'+π4.ifx<x1

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

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