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Find the (lowest order) relativistic correction to the energy levels of the one-dimensional harmonic oscillator. Hint: Use the technique in Example 2.5 .

Short Answer

Expert verified

The lowest-order relativistic correction to the energy levels is

Er1=-32ω232mc2(2n2+2n+1)

Step by step solution

01

relativistic correction to the energy levels

The relativistic correction to the energy levels is:

Er1=-12mc2[En2-2EnV^+V^2]

For the harmonic oscillator

V^=12mω2x2^En=ω(n+12)

02

write the relativistic correction to the energy as

Now, we can write the relativistic correction to the energy as:

Er1=-12mc22ω2n+122-2ωn+1212ωn+12+14m2ω4x^4

From the example (2.5), we get:

x^2=2mωa+a++a+a+aa++aaV^=12ωn+12

Then

Er1=-12mc22ω2n+122-2ω2n+122+14m2ω4x^4

03

find ⟨x^4⟩

We need to find x^4by calculating that:

x^4=24m2ω2(a+a++a+a+aa++aa)(a+a++a+a+aa++aa)x^4=n|x^4|n=24m2ω2[n|a+a+a+a+|n+n|a+a+a+a|n+n|a+a+aa+|n+n|a+a+aa|n+n|a+aa+a+|n+n|a+aa+a|n+n|a+aaa+|n+n|a+aaa|n+n|aa+a+a+|nn+n|aa+a+a|n+n|aa+aa+|n+n|aa+aa|n+n|aaa+a+|n+n|aaa+a|n+n|aaaa+|n+n|aaaa|n

We know that:

a+|n=n+1|n+1a|n=n|n-1

Where, the terms which contain equal number particles due to the raising and lowering operators can survive and the other terms equal to zero fromδnm=0;nm

04

calculate the terms which are required in above equation

Then, the only terms which can be calculated are:

n|a+a+aa|n=nn|a+a+a|n-1=n(n-1)n|a+a+|n-2=n(n-1)n|a+|n-1=n(n-1)nn=n(n-1)δnn=n(n-1)

Solve further

n|a+aa+a|n=nn|a+aa+|n-1=nn|a+a|n=nnn|a+|n-1=n2nn=n2δnn=n2n|a+aaa+|n=(n+1)n|a+aa|n+1=(n+1)n|a+a|n=n(n+1)n|a+|n-1=n(n+1)nn=n(n+1)δnn

Solve further

=n(n+1)n|aa+a+a|n=nn|aa+a+|n-1=nn|aa+|n=n(n+1)n|a|n+1=n(n+1)nn=n(n+1)δnn=n(n+1)=(n+1)n|aa+|n

Solve further

=(n+1)(n+1)n|a|n+1=(n+1)2nn=(n+1)2δnn=(n+1)2|aaa+a+|n=(n+1)n|aaa+|n+1=(n+1)(n+2)n|aa|n+2=(n+2)(n+1)n|a|n+1=(n+1)(n+2)nn=(n+1)(n+2)δnn=(n+1)(n+2)

05

solve for ⟨x^4⟩

Then,

x^4=24m2ω2n(n-1)+n2+n(n+1)+n(n+1)+(n+1)2+(n+1)(n+2)=24m2ω2n2-n+n2+n2+n+n2+n+n2+2n+1+n2+2n+n+2=24m2ω2[6n2+6n+3]

06

calculate the correction in the energy levels

Now we can calculate the correction in the energy levels:

Er1=-12mc214m2ω424m2ω2(6n2+6n+3)=-2ω232mc2(6n2+6n+3)

Then, the lowest-order relativistic correction to the energy levels is

Er1=-32ω232mc2(2n2+2n+1)

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Most popular questions from this chapter

Suppose we put a delta-function bump in the center of the infinite square well:

H'=αδ(x-a/2)

whereais a constant.

(a) Find the first-order correction to the allowed energies. Explain why the energies are not perturbed for evenn.

(b) Find the first three nonzero terms in the expansion (Equation 6.13) of the correction to the ground state,Ψ11.

Consider a particle of mass m that is free to move in a one-dimensional region of length L that closes on itself (for instance, a bead that slides frictionlessly on a circular wire of circumference L, as inProblem 2.46).

(a) Show that the stationary states can be written in the formψn(x)=1Le2πinx/L,(-L/2<x<L/2),

wheren=0,±1,±2,....and the allowed energies areEn=2mnπL2.Notice that with the exception of the ground state (n = 0 ) – are all doubly degenerate.

(b) Now suppose we introduce the perturbation,H'=-V0e-x2/a2where aLa. (This puts a little “dimple” in the potential at x = 0, as though we bent the wire slightly to make a “trap”.) Find the first-order correction to En, using Equation 6.27. Hint: To evaluate the integrals, exploit the fact that aLato extend the limits from ±L/2to±after all, H′ is essentially zero outside -a<x<a.

E±1=12Waa+Wbb±Waa-Wbb2+4Wab2(6.27).

(c) What are the “good” linear combinations ofψnandψ-n, for this problem? Show that with these states you get the first-order correction using Equation 6.9.

En'=ψn0H'ψn0(6.9).

(d) Find a hermitian operator A that fits the requirements of the theorem, and show that the simultaneous Eigenstates ofH0and A are precisely the ones you used in (c).

Question: Consider a quantum system with just three linearly independent states. Suppose the Hamiltonian, in matrix form, is

H=V0(1-o˙0000o˙0o˙2)

WhereV0is a constant, ando˙is some small number(1).

(a) Write down the eigenvectors and eigenvalues of the unperturbed Hamiltonian(o˙=0).

(b) Solve for the exact eigen values of H. Expand each of them as a power series ino˙, up to second order.

(c) Use first- and second-order non degenerate perturbation theory to find the approximate eigen value for the state that grows out of the non-degenerate eigenvector ofH0. Compare the exact result, from (a).

(d) Use degenerate perturbation theory to find the first-order correction to the two initially degenerate eigen values. Compare the exact results.

Calculate the wavelength, in centimeters, of the photon emitted under a hyperfine transition in the ground state (n=1) of deuterium. Deuterium is "heavy" hydrogen, with an extra neutron in the nucleus; the proton and neutron bind together to form a deuteron, with spin 1 and magnetic moment

μdl=gde2mdSd

he deuteron g-factor is 1.71.

Problem 6.6 Let the two "good" unperturbed states be

ψ±0=α±ψa0+β±ψb0

whereα±andβ±are determined (up to normalization) by Equation 6.22(orEquation6.24). Show explicitly that

(a)are orthogonal;role="math" localid="1655966589608" (ψ+0ψ-0=0);

(b) ψ+0|H'|ψ-0=0;

(c)ψ±0|H'|ψ±0=E±1,withE±1given by Equation 6.27.

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