Physics Problem Solution: Eigenvalues & Eigenvectors of Perturbed Symmetrical Matrix, Assignments of Quantum Physics

A solution to a physics problem involving the calculation of eigenvalues and eigenvectors of a symmetrical matrix, as well as the application of perturbation theory. The problem discusses the effect of a delta-function bump on the infinite square well potential and the resulting correction to the energy levels.

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Pre 2010

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Physics 487 Discussion 4 September 20, 2005
Solution
1. (I’ve deleted the preamble and footnotes.)
On the way to the complete BCS theory, Cooper proposed that
ˆ
U
is very symmetrical: all of
its matrix elements are equal. This means that
ˆ
U
is a very simple R×R matrix:
ˆ
U=!a
1!1!1
" # $ "
111
" $ # "
1!1!1
"
#
$
$
$
$
$
$
%
&
'
'
'
'
'
'
.
This problem can be solved exactly. Calculate the eigenvalues of
ˆ
U
. You will find that one
eigenvalue is special. What is its eigenvector?
Hint: Some properties of eigenvalue problems may be helpful:
The sum of the diagonal elements (the trace) = the sum of the eigenvalues.
The sum of the squares of all the matrix elements = the sum of the squares of the
eigenvalues. (I think this may only hold for Hermitian operators.)
The determinant of the matrix = the product of the eigenvalues.
The equality of rows means the determinant = 0. Therefore, at least one eigenvalue = 0. In
fact, it’s easy to write down R-1 eigenvectors that all have ε = 0:
(1, -1, 0, 0, ... 0), (1, 0, -1, 0, ... 0), ... (1, 0, 0, 0, ... -1)
I haven’t chosen an orthonormal set of eigenvectors, but that’s not important here.
The trace of the matrix = -Ra, so Rth eigenvalue must equal -Ra. The eigenvector is
(1, 1, 1, 1 ... 1). Note that it is orthogonal to all of the others (because it has a different
eigenvalue).
So, we have an energy spectrum with a big gap:
In a macroscopic material, R can be very large, so the
gap can be big even if a is very small. Only the single
ground state will be affected by BEC.
R-1 degenerate
states
1 state
Ra
pf3

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Physics 487 Discussion 4 September 20, 2005

Solution

1. (I’ve deleted the preamble and footnotes.)

On the way to the complete BCS theory, Cooper proposed that

U is very symmetrical: all of

its matrix elements are equal. This means that

U is a very simple R × R matrix:

U =! a

This problem can be solved exactly. Calculate the eigenvalues of

U. You will find that one

eigenvalue is special. What is its eigenvector?

Hint: Some properties of eigenvalue problems may be helpful:

  • The sum of the diagonal elements (the trace) = the sum of the eigenvalues.
  • The sum of the squares of all the matrix elements = the sum of the squares of the

eigenvalues. (I think this may only hold for Hermitian operators.)

  • The determinant of the matrix = the product of the eigenvalues.

The equality of rows means the determinant = 0. Therefore, at least one eigenvalue = 0. In

fact, it’s easy to write down R - 1 eigenvectors that all have ε = 0:

I haven’t chosen an orthonormal set of eigenvectors, but that’s not important here.

The trace of the matrix = - Ra , so R

th eigenvalue must equal - Ra. The eigenvector is

(1, 1, 1, 1 ... 1). Note that it is orthogonal to all of the others (because it has a different

eigenvalue).

So, we have an energy spectrum with a big gap:

In a macroscopic material, R can be very large, so the

gap can be big even if a is very small. Only the single

ground state will be affected by BEC.

R - 1 degenerate

states

1 state

Ra

2. This is Griffiths, problem 6.1 (page 254).

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

H

'

= !" ( x # a / 2 ) , where α is a constant.

a. Find the first order correction to the allowed energies. Explain why the energies are not

perturbed for even n.

The unperturbed wave functions are! n

( x ) =^

2

a

sin

n " x

a

The first order correction to each energy is:

E

n

1 =! " n

( x )

2

0

a

$ ( x % a / 2 ) dx =! "

n

( a / 2 )

2

=

2!

a

for odd n

0 for even n

Perturbations at nodes don’t have 1

st order effects. There might be higher order effects.

b. Find the first three nonzero terms in the 1

st order correction to the ground state,! 1

1 :

n

1

m

H

' n

0

E

n

0 ! E m

0

m

0

m " n

where m

0 is the unperturbed m

th state, and n

1 is the n

th state after the first

perturbation correction.

We must calculate the matrix elements of

H

' :

m

0 ˆ H

' 1

0

a

sin

m " x

a

sin

" x

a

) ( x * a / 2 ) dx

0

a

a

sin

m "

Only the odd m terms are nonzero, so the first three nonzero terms in 1

1 are:

1

4 2! ma

2

a

3 2 "

2 !

2

2

sin

3 " x

a

2

sin

5 " x

a

2

sin

7 " x

a

I used E n

0

n

2 !

2 !

2

2 ma

2

, the unperturbed energies.