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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

Short Answer

Expert verified

The bond state energy of hydrogen E is,

E=-13.6eVn-12+II+12

Step by step solution

01

Using radial equation of hydrogen. 

The radial equation for hydrogen is given by:

h22md2udr2+-e24πO01r+h22mII+1r2u=Eu

Where u(r)=rR(r) and the effective potential is the terms inside the square brackets, that is:

Vr=-e24πO01r+h22mII+1r2

In this case we have two turning points,r1andr2at both sides of the well, these two points can be determined by setting the potential equal to the energy, so the two turning points are the roots of:

E=-e24πO01r+h22mII+1r2 ……………….(1)

The WKB equations satisfy the condition:

r1T2prdr=n-12πh …………………..(2)

Now we need to find the integral in (2), where ,pr=2mE-V, so we have:

r1f2prdr=2mr1f2E+e24πο01r-h22mII+1r2drr1f2prdr=-2mEr1f21r-r2-e24πο0Er+h22mEII+1dr

In the second line we factored out -E . The equation under the square root is identical to equation (1), so the solutions of the equation are r1and r2. To simplify, we let:

B=-e24πο0EC-h22mEII+1

02

To find the integral value.

Thus,

τ1r2prdr=-2mEr1r21r-r2+Br-Cdr

As we said before, the solutions of the equation under the square root are the two turning points r1and r2, which are given by the general law, as:

r1=B-B2-4C2r2=B2-4C2

So we can write:

-r2+Br-C=r-r1r2-r

Thus,

r1r2prdr=-2mEr1f2r-r1r2-rdrr1r2prdr=-2mEπ2r2-r12r1r2prdr=-2mEπ2r1+r2-2r1r2r1r2prdr=-2mEπ2B-2C

r1r2prdr=-2mEπ2-e24πο0E-2-h22mEII+1r1r2prdr=π2-e22m4πο0-E-2hII+1

Where in the second line, I used the given integral in the problem.

Substitute into (2) to get:

π2-e22m4πο0-E-2hII+1=n-12πh

Solve for E as:

-e22m4πο0-E-2hII+1=2n-1h-e22m4πο0-E=2n-1h+2hII+1E=e24πο0m2h2n-12+II+12

03

By using Bohr formula to find bound state energy of hydrogen.

Thus,

E=E0n-12+II+12

Where is the ground state energy of the hydrogen atom, and it is given by the Bohr formula:

E0=-e24πο02m2h2E0=13.6eV

Thus,

E=-13.6eVn-12+II+12.

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Most popular questions from this chapter

Analyze the bouncing ball (Problem 8.5) using the WKB approximation.
(a) Find the allowed energies,En , in terms of , and .
(b) Now put in the particular values given in Problem8.5 (c), and compare the WKB approximation to the first four energies with the "exact" results.
(c) About how large would the quantum number n have to be to give the ball an average height of, say, 1 meter above the ground?

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 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 .

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> .

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