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 .

Short Answer

Expert verified

The energy of the harmonic oscillator is,

En=αn-12ħΓ1v+32Γ1v+1π2mα2vv+2

Step by step solution

01

To find the allowed energies of potential. 

In this problem we need to use the WKB approximation to find the allowed energies of the potential

Vx=αxv………………….(1)

Where αand v are positive constants, when we apply the WKB approximation to a potential well in problem 8.1, we get the condition

x1x2pxdx=n-12πħ …………………(2)

Where x1is the left turning point, x2is the right turning point. At the turning point the values of the energy equal the potential, so to find these points we set E=V(x) , so we get:

x1,2=±Eα1/vSotheintegralin(2)willbe:x1x2pxdx=-(EIα)1/VEIα1/V2mE-αxvdxx1x2pxdx=0(EIα)1/V2mE-αxvdxUsingthesubstitution,u=xvdu=vx1-1/vdxdu=νu1-1/vdx

dx=1vu1/v-1duNowtheturningpointinisE/α,thus:x1x2pxdx=20E/α1/22m(E-αxv)dxx1x2p(x)dx=22mv0E/αE-αuu1/v-1du

02

To find an integral.

Using any program we can find the integral, I used Mathematical to do so, and I got:

0E/αE-αuu1/v-1du=π2α1/vΓ1vΓ1v+32E1v+1vThus,x1x2pxdx=2πmv1α1/vΓ1vΓ1v+32E1v+1vUsing(2)weget,2πmv1α1/vΓ1vΓ1v+32E1v+1v=n-12πħSolveforE,Env+22v=n-12πħΓ1v+32Γ1v1/v2πmEn=n-12πħΓ1v+32Γ1v1/v2πm2vv-2

role="math" localid="1656055283739" UsingtheidentityΓz+1=z,soweget:En=n-12πħΓ1v+32Γ1v+1α1/v2πm2vv-2Wealsohave:α1/v2vv+2=α2vv+2α1/v2vv+2=αv+2-vv+2α1/v2vv+2=α.α-vv+2α1/v2vv+2=α.α-1/22vv+2

03

By using harmonic oscillator formula to find energies.

Thus,

En=αn-12ħΓ1v+32Γ1v+1π2mα2vv+2 ……………………(3)

Now we need to check this formula for the harmonic oscillator case, with a potential of:

Vx=12mω2x2

Compare it with equation (1), we get v=2 and α=12mω2, so we need

Γ2=1Γ32=12πtoget,En=n-12ħωwhichistheenergyoftheharmonicoscillator.

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Most popular questions from this chapter

Use equation 8.22 calculate the approximate transmission probability for a particle of energy E that encounters a finite square barrier of height V0 > E and width 2a. Compare your answer with the exact result to which it should reduce in the WKB regime T << 1.

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> .

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

Use the WKB approximation to find the allowed energies (En)of an infinite square well with a “shelf,” of heightV0, extending half-way across

role="math" localid="1658403794484" V(x)={v0,(0<x<a/2)0,(a/2<x<a),(otherwise)

Express your answer in terms ofrole="math" localid="1658403507865" V0andEn0(nπħ)2/2ma2(the nth allowed energy for the infinite square well with no shelf). Assume that, but do not assume that E10>V0. Compare your result with what we got in Section 7.1.2, using first-order perturbation theory. Note that they are in agreement if eitherV0is very small (the perturbation theory regime) or n is very large (the WKB—semi-classical—regime).

Use the WKB approximation in the form

r1r2p(r)dr=(n-1/2)πh

to estimate the bound state energies for hydrogen. Don't forget the centrifugal term in the effective potential (Equation ). The following integral may help:

ab1x(x-a)(b-x)dx=π2(b-a)2.

Note that you recover the Bohr levels whenn/andn1/2

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