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.

Short Answer

Expert verified

The answers are

a)v1=100,V0;v2=010,V0;v3=001,2V0

b)role="math" localid="1658144006650" λ1=V0(1-o˙),λ2=V023-4o˙2V0(1-o˙2),λ3=V023+4o˙2V0(2-o˙2)

c)E31=0,E32,=o˙2V0

d)E1=V0-o˙V0,E2=V01+

Step by step solution

01

Cigen vector and eigen values of Hamiltonian

a)

In this problem we study the Hamiltonian

H=V01-o˙0000o˙0o˙2

The unperturbed Hamiltonian is obtained by settingo˙=0 and is of the form

Since it is diagonal, its Eigen values are

V0,V0,2V0

And

the eigenvectors are

V1=100V2=010V3=001

02

Expand eigen values as power series of H

b)

We now diagonalize the total Hamiltonian by solving the equation

V0(1-o˙)-λ000V0-λV0o˙0V0o˙2V0-λ=0(V0(1-o˙)-λ)(V0-λ)(2V0-λ)-V02o˙2(V0(1-o˙)-λ)=0(V0(1-o˙)-λ)(V0-λ)(2V0-λ)-V02o˙2=0

The one eigen value is

λ1=V0(1-o˙)

and the other two are obtained as

λ2-3V0λ+V0(2-o˙2)=0λ2,3=123V0±9V02-4V02(2-o˙2)=V023±1+4o˙2

We can expand these Eigen values with respect to to obtain

λ1=V0(1-o˙),λ2=V023+1+4o˙2V02(3+1+2o˙2)=V02+o˙2λ3=V023-1+4o˙2V02(3-1-2o˙2)=V01-o˙2

We have used the Taylor expansion of the square root 1+o˙1+o˙/2.

03

Find approximate eigen values for state

c)

We now observe the perturbed part of the Hamiltonian

H=o˙V0-100001010

By settingo˙=0we see that λ1=λ2, so we are calculating the corrections for E3. The first-order correction is

The second-order corrections are

E32=m-12vmHv32E30-Em0

We have

localid="1658203255352" vmHv3=o˙V0(100)-100001010001=0vmHv3=o˙V0(010)-100001010001=o˙V0E30-E20=2V0-V0=V0

Therefore,

Ea2=o˙V02V0=o˙2V0

The total energy is then

E3=E30+E31+E32=2V0+0+o˙2V0=V02+o˙2

which is what we obtained by expanding the exact solution.

04

First order eigen values for degenerate state

d)

We now calculate the corrections to the degenerate energies. We have

Waa=v1Hv1=o˙V0(100)-100001010100=-o˙V0Wbb=v2Hv2=o˙V0(010)-100001010010=0Wab=v1Hv2=o˙V0(100)-100001010010=0E30-E20=2V0-V0=V0

The energies are

E±1=12Waa+Wbb±Waa-Wbb2+4Wab2=12Waa±Waa=12-o˙Va±o˙V0

The energies corrections are

E-=-o˙V0,E+=0

and the energies are

E1=V0-o˙V0,E2=V0

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Most popular questions from this chapter

Question: In a crystal, the electric field of neighbouring ions perturbs the energy levels of an atom. As a crude model, imagine that a hydrogen atom is surrounded by three pairs of point charges, as shown in Figure 6.15. (Spin is irrelevant to this problem, so ignore it.)

(a) Assuming that rd1,rd2,rd3show that

H'=V0+3(β1x2+β2y2+β3z2)-(β1+β2+β3)r2

where

βi-e4πε0qidi3,andV0=2(β1d12+β2d22+β3d32)

(b) Find the lowest-order correction to the ground state energy.

(c) Calculate the first-order corrections to the energy of the first excited states Into how many levels does this four-fold degenerate system split,

(i) in the case of cubic symmetryβ1=β2=β3;, (ii) in the case of tetragonal symmetryβ1=β2β3;, (iii) in the general case of orthorhombic symmetry (all three different)?

Van der Waals interaction. Consider two atoms a distanceapart. Because they are electrically neutral you might suppose there would be no force between them, but if they are polarizable there is in fact a weak attraction. To model this system, picture each atom as an electron (mass m , charge -e ) attached by a spring (spring constant k ) to the nucleus (charge +e ), as in Figure. We'll assume the nuclei are heavy, and essentially motionless. The Hamiltonian for the unperturbed system is

H0=12mp12+12kx12+12mp22+12kx22[6.96]

The Coulomb interaction between the atoms is

H'=14πϵ0(e2R-e2R-x1-e2R+x2+e2R-x1+x2 [6.97]

(a) Explain Equation6.97. Assuming that localid="1658203563220" |x1| and |x2|are both much less than, show that

localid="1658203513972" H'-e2x1x22πϵ0R3 [6.98]

(b) Show that the total Hamiltonian (Equationplus Equation) separates into two harmonic oscillator Hamiltonians:

H=[12mp+2+12(k-e22πϵ0R3x+2]+[+12mp-2+12(k+e22πϵ0R3x-2] [6.99]

under the change of variables

x±12(x1±x2) Which entails p±=12(p1±p2) [6.100]

(c) The ground state energy for this Hamiltonian is evidently

E=12(ω++ω-) Where ω±=k(e2/2πϵ0R3)m [6.101]

Without the Coulomb interaction it would have been E0=ħω0, where ω0=k/m. Assuming that, show that

ΔVE-E0-8m2ω03(e22πϵ0)21R6. [6.102]

Conclusion: There is an attractive potential between the atoms, proportional to the inverse sixth power of their separation. This is the van der Waals interaction between two neutral atoms.

(d) Now do the same calculation using second-order perturbation theory. Hint: The unperturbed states are of the form ψn1(x1)ψn2(x2), where ψn(x)is a one-particle oscillator wave function with mass mand spring constant k;ΔVis the second-order correction to the ground state energy, for the perturbation in Equation 6.98 (notice that the first-order correction is zero).

Prove Kramers' relation:

sn2rs-(2s+1)ars-1+s4[(2l+1)2-s2]a2rs-2=0

Which relates the expectation values of rto three different powers (s,s-1,ands-2),for an electron in the state ψn/mof hydrogen. Hint: Rewrite the radial equation (Equation) in the form

u''=[l(l+1)r2-2ar+1n2a2]u

And use it to expressrole="math" localid="1658192415441" (ursu'')drin terms of (rs),(rs-1)and(rs-2). Then use integration by parts to reduce the second derivative. Show that (ursu'')dr=-(s/2)(rs-1)and(u'rsu')dr=-[2/s+1](u''rs+1u')dr. Take it from there.

The Feynman-Hellmann theorem (Problem 6.32) can be used to determine the expectation values of1/rand1/r2for hydrogen.23The effective Hamiltonian for the radial wave functions is (Equation4.53)

22md2dr2+22ml(l+1)r2-e24π01r

And the eigenvalues (expressed in terms ofl)24are (Equation 4.70)

En=-me432π202h2jmax+l+12

(a) Use λ=ein the Feynman-Hellmann theorem to obtain 1/r. Check your result against Equation 6.55.

(b) Use λ=lto obtain 1/r2. Check your answer with Equation6.56.

Starting with Equation 6.80, and using Equations 6.57, 6.61, 6.64, and 6.81, derive Equation 6.82.

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