- •General aspects
- •Introduction
- •Single particle
- •General aspects
- •Traps
- •Many particles
- •Basics of second quantization
- •Bosons
- •Fermions
- •Single particle operator
- •Two particle operator
- •Bosons
- •Free Bose gas
- •General properties
- •BEC in lower dimensions
- •Trapped Bose gas
- •Parabolic trap
- •Weakly interacting Bose gas
- •BEC in an isotr. harmonic trap at T=0
- •Comparison of terms in GP
- •Thomas-Fermi-Regime
- •Fermions
- •Free Fermions
- •General properties
- •Pressure of degenerated Fermi gas
- •Excitations of Fermions at T=0
- •Trapped non-interacting Fermi gas at T=0
- •Weakly interacting Fermi gas
- •Ground state
- •Decay of excitations
- •Landau-Fermi-Liquid
- •Zero Sound
- •Bardeen-Cooper-Shieffer-Theory
- •General treatment
- •BCS Hamiltonian
- •General energy-momentum relation
- •Calculation for section 3.3.1
- •Lifetime and Fermis Golden Rule
- •Bibliography
70 |
|
|
|
|
|
|
|
|
|
|
CHAPTER 3. FERMIONS |
which leads to |
|
|
|
|
|
|
|
|
|
||
1 |
|
2 |
|
1 |
|
|
|
|
|||
|
|
ln |
|
|
|
= |
|
|
+ 1 |
(3.199) |
|
|
2 |
e |
F0 |
||||||||
|
|
|
|
|
|
2 |
|
|
2 |
|
|
|
|
|
) e = |
|
e F0 |
(3.200) |
|||||
|
|
|
e2 |
This is a collective mode in a degenerated collisionless regime (zero sound) with the velocity
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
2 |
|
|
2 |
|
|
|
|
|
|
||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
c0 = vF |
|
|
1 + |
|
|
e F0 vF |
|
|
|
|
(3.201) |
|||||||||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
e2 |
|
|
|
|
||||||||||||||||||||||||||
compared to sound in the hydrodynamic regime: |
|
|
|
|
|
|||||||||||||||||||||||||||||||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
0 |
|
|
|
|
|
|
1 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||
|
|
¶p |
|
|
|
|
1 ¶p |
1 |
|
|
¶ |
|
|
|
2 |
|
3 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||||||||||||
c12 = |
|
|
|
|
|
= |
|
|
|
|
|
= |
|
|
|
|
B |
|
n |
|
eFC |
|
|
|
|
(3.202) |
||||||||||||||||||||
¶r |
m |
¶n |
m |
¶n |
3 |
5 |
|
|
|
|
||||||||||||||||||||||||||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
B |
|
|
E |
C |
|
|
|
|
|
||||||||||||||
|
1 |
|
|
|
|
|
|
|
|
2 |
|
1 6 |
@ |
|
|
2 |
|
|
|
A |
6 |
2 |
3 |
|
2 |
|||||||||||||||||||||
|
|
|
|
|
|
0 |
|
2 |
3 |
|
|
|{z}3 |
1 5 1 1 |
|
n |
3 |
||||||||||||||||||||||||||||||
= m ¶n |
5 n 2m |
pg~ |
|
|
n |
1 |
|
= m 3 5 m |
|
pg~ |
|
(3.203) |
||||||||||||||||||||||||||||||||||
|
|
|
|
|
|
|
@ |
|
|
|
|
|
|
|
|
|
|
|
|
|
A |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||||
|
|
¶ |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||||||||||||||||||||||
|
1 |
|
|
|
|
|
2 |
|
|
2 |
|
|
|
|
|
|
|
|
|
|
|
|
vF |
|
|
|
|
|
||||||||||||||||||
|
|
|
|
pF |
|
|
|
vF |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||||||||||||||||
= |
|
|
|
|
= |
|
|
|
|
|
|
|
|
) |
|
|
|
|
|
c1 = p |
|
|
|
|
|
|
(3.204) |
|||||||||||||||||||
3 |
m |
3 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||||||||||||||||||||||||||||
|
|
|
|
|
|
|
|
|
|
|
3 |
|
|
|
|
|||||||||||||||||||||||||||||||
This is ordinary hydrodynamic sound. |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
If F0 was negative s became a complex number with real and imaginary parts being of the same order. Hence, in this case the collective mode is overdamped and of no interest.
3.5 Bardeen-Cooper-Shieffer-Theory
3.5.1 General treatment
If we consider two FERMIons in vacuum we have a simple quantum mechanical problem. We use the frame of reference where the center of mass is at rest:
|
|
|
|
|
|
|
~ |
|
|
|
|
|
(3.205) |
|
|
|
|
|
|
|
|
P = ~p1 +~p2 = 0 |
|
|
|
||||
Here we can write the SCHRÖDINGER |
equation as |
|
|
|
|
|
||||||||
|
~2 |
|
2 |
2 |
|
|
|
y(~r1 |
|
|
|
|
|
|
|
Ñ1 |
+ Ñ2 |
+UI |
~r1 ~r2 |
;~r2) = Ey(~r1;~r2) |
(3.206) |
||||||||
2m |
||||||||||||||
|
|
|
|
|
|
|
|
|
~p(~r1 |
|
~r2) |
|||
|
|
|
|
|
|
|
|
y(~r1 |
;~r2) = åc~pe |
i |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||||
|
|
|
|
|
|
|
|
|
~ |
(3.207) |
||||
|
|
|
|
|
|
|
|
|
|
|
~p
3.5. BARDEEN-COOPER-SHIEFFER-THEORY |
71 |
i.e. we decompose the wave function into plane waves. Inserting this decomposition we get the SCHRÖDINGER equation in momentum space
(e1 + e2)c~p + åUI(~p ~p 0)c~p 0 |
= Ec~p |
(3.208) |
||||||
|
|
~p 0 |
|
|
|
|
|
|
where |
|
|
|
|
|
|
|
|
|
|
|
|
|
p2 |
|
|
|
e1 = e2 = |
|
= ep |
|
(3.209) |
||||
|
|
|||||||
|
|
|
|
|
2m |
|
|
|
since both particles are identical. |
Rewriting the SCHRÖDINGER |
equation once |
||||||
more we have |
|
|
|
|
|
|
|
|
(E 2ep)c~p = åUI(~p ~p 0)c~p 0 |
or |
(3.210) |
||||||
|
~p 0 |
|
|
|
|
|
|
|
c~p = |
|
1 |
|
|
åUI(~p ~p 0)c~p 0 |
(3.211) |
||
E |
2 |
|
|
|||||
|
|
|
ep ~p 0 |
|
|
This discussion is still exact. Now we use a model for the interatomic potential
U |
p |
|
p |
|
|
|
|
V0 |
¯ |
(3.212) |
||
|
|
|
|
|
0 ep;ep0 w |
|||||||
I |
(~ |
~ 0) = |
(0 |
|
otherwise |
|
||||||
In ordinary space this expression looks rather strange. |
|
|||||||||||
Using this model we have |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
1 |
|
|
¯ |
|
˜ |
|
||
c~p |
= E |
|
2 |
|
|
(3.213) |
||||||
|
|
|
Θ(w |
ep)V0åc~p 0 |
||||||||
|
|
|
|
|
ep |
|
~p 0 |
|
||||
The tilde denotes that the sum obeys the constraint |
|
|||||||||||
|
|
|
|
|
|
|
ep0 w¯ |
(3.214) |
||||
To solve this expression, we sum over all coefficients |
|
|||||||||||
|
|
˜ |
|
|
|
|
˜ |
1 ˜ |
|
|||
|
åc~p |
= V0å |
|
|
åc~p 0 |
(3.215) |
||||||
|
|
|
||||||||||
|
|
~p |
|
|
|
|
~p E 2ep ~p 0 |
|
||||
|
|
|
|
|
|
|
|
˜ |
1 |
|
|
|
|
|
, 1 = V0å~p |
|
|
(3.216) |
|||||||
|
|
E 2ep |
Since we are looking at an attractive interaction and more specifically for bound states we have
V0 = jV0j E = 2 |
(3.217) |
72 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
CHAPTER 3. FERMIONS |
||||||||
where is the binding energy per particle. Using this we have |
|
||||||||||||||||||||||||||||||||||||||||||||
|
1 |
|
|
˜ |
1 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||||
1 = |
|
|
jV0jå |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
(3.218) |
||||||
2 |
|
+ ep |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||||||||||||
|
|
|
|
|
~p |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|||
|
1 |
|
¯ |
|
|
|
|
|
|
|
|
|
|
|
|
|
1 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||
|
|
|
|
w |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||
= |
|
|
jV0jZ0 |
de n(e) |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
(3.219) |
|||||||||||||||
2 |
|
|
+ e |
|
|
|
|
|
|
|
|
|
|
||||||||||||||||||||||||||||||||
|
1 |
|
|
|
w¯ |
|
|
mp |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
1 |
|
|
|
|
|
|
|
|
|
|
||||||||||
|
|
|
|
2m |
|
|
|
|
|
|
|
|
|||||||||||||||||||||||||||||||||
= |
|
|
jV0jZ0 |
de |
|
|
|
|
|
|
|
|
|
|
pe |
|
|
|
|
|
|
|
|
|
|
|
|
(3.220) |
|||||||||||||||||
2 |
2p2~3 |
|
|
+ e |
|
|
|
|
|
|
|
||||||||||||||||||||||||||||||||||
|
|
|
mp |
|
|
Z0 |
p |
|
|
|
|
|
|
|
|
|
|
|
2x2 |
|
|
|
|
|
|
|
|
||||||||||||||||||
= |
1 |
|
2m |
|
w¯ |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
(3.221) |
||||||||||||||||||||||||
|
jV0j |
|
|
|
|
|
|
|
|
|
dx |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||||||||||||||
2 |
2p2~3 |
|
|
|
|
|
|
|
|
+ x2 |
|
|
|
|
|
|
|
||||||||||||||||||||||||||||
|
|
|
|
mp |
|
|
|
p |
|
|
|
|
|
|
|
1 |
|
|
|
|
|
|
|||||||||||||||||||||||
|
|
|
|
m |
|
|
w¯ |
|
|
|
|
|
1 |
|
|
||||||||||||||||||||||||||||||
= jV0j |
2 |
Z0 |
|
|
|
dx |
|
|
|
|
|
|
(3.222) |
||||||||||||||||||||||||||||||||
2p2~3 |
|
|
|
|
|
|
+ x2 |
|
|||||||||||||||||||||||||||||||||||||
|
|
|
|
mp |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
p |
|
|
|
|
|
|
|||||
|
|
|
|
m |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
¯ |
|
|
||||||||||
= jV0j |
2 |
pw¯ p |
|
|
arctan p |
w |
|
|
(3.223) |
||||||||||||||||||||||||||||||||||||
2p2~3 |
|||||||||||||||||||||||||||||||||||||||||||||
|
|
||||||||||||||||||||||||||||||||||||||||||||
|
|
|
|
mp |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
p |
|
|
|
|
|
|
|
|
|
|
|
|
||||||||||||
|
|
|
|
2m |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||||||||||
jV0j |
|
npw¯ |
|
|
|
|
p |
o |
|
|
|
|
|
|
|
(3.224) |
|||||||||||||||||||||||||||||
2p2~3 |
|
|
2 |
|
|
|
|
|
|
|
|||||||||||||||||||||||||||||||||||
= jV0jn(w¯)(1 |
2 r |
|
|
|
) |
|
|
|
|
|
|
|
|
|
|
(3.225) |
|||||||||||||||||||||||||||||
w¯ |
|
|
|
|
|
|
|
|
|
|
|||||||||||||||||||||||||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
p |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
Here we assumed that w¯ and thus the arcus tangent can be approximated as p2 . Solving this we have
r
|
|
2 |
|
|
1 |
|
|
|
|
|
= |
|
1 |
|
|
> 0 |
(3.226) |
||
¯ |
|
|
V ( |
) |
|||||
w |
p |
|
j |
0jn eF |
|
|
|
Therefore we have threshold (i.e. a minimal jV0j) before a bound state appears. Now we want to consider two FERMIons on top of a filled and frozen F ERMI sphere. Frozen means that we will not consider interactions of the particles inside the FERMI sphere with our two extra particles. In this case we have
ep;ep0 eF |
|
|
|
|
|
|
|
|
|
(3.227) |
|
c~p = |
1 |
|
|
~p |
0 |
cp |
|
(3.228) |
|||
|
~p 0 ~pF |
0 |
|||||||||
E 2ep |
|||||||||||
|
å |
UI ~p |
|
|
|
|
|||||
We assume for the potential |
|
|
|
|
|
|
|
|
|
|
|
I(~ ~ 0) = (0 |
otherwise |
|
|
|
|
|
|
¯ |
|
||
U p p |
V0 |
eF ep;ep0 |
eF + w |
(3.229) |
3.5. BARDEEN-COOPER-SHIEFFER-THEORY |
|
|
73 |
|||||||||||||||
Now we define |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
xp = ep eF 0 |
|
|
(3.230) |
||||||||||
and note that the energy of the ground state is now |
|
|
|
|||||||||||||||
|
|
|
|
|
|
E = 2eF 2 |
|
|
|
(3.231) |
||||||||
where is the binding energy per particle. |
|
|
|
|
|
|
|
|
||||||||||
Again we can rewrite the SCHRÖDINGER |
|
equation in our case as |
|
|||||||||||||||
|
|
|
|
|
¯ |
|
|
|
|
|
|
|
|
|
|
|||
|
|
|
c |
= |
Θ(w xp) |
V |
˜ c |
|
|
(3.232) |
||||||||
|
|
|
~p |
|
2( + x |
) j |
0jå ~p 0 |
|
|
|
||||||||
|
|
|
|
|
|
|
|
|
|
p |
|
|
|
|
~p 0 |
|
|
|
|
|
|
¯ |
|
¯ |
|
|
|
|
|
|
|
|
|
|
|
||
The tilde denotes xp0 w. |
|
|
|
|
|
|
|
|
|
|
|
|||||||
Using the same method with |
w eF as before we get |
|
||||||||||||||||
|
1 |
˜ |
1 |
|
1 |
|
|
¯ |
|
|
|
|
|
1 |
|
|
||
|
|
|
w |
|
|
|
|
|
|
|
||||||||
1 = |
|
jV0jå~p |
|
|
= |
|
jV0jZ0 |
|
|
dx n(eF + xp) |
|
|
(3.233) |
|||||
2 |
+ xp |
2 |
|
|
+ xp |
|||||||||||||
|
2 jV0jn(eF)ln |
+ w |
2 jV0jn(eF)ln w |
(3.234) |
||||||||||||||
|
1 |
|
|
|
¯ |
|
1 |
|
|
|
|
¯ |
|
|
||||
In the last step we approximated again |
|
|
¯ |
|
|
|
|
|||||||||||
w |
. solving this for the binding energy |
we see, that there is always a solution regardless of the strength of the potential
= we |
|
2 |
|
C |
|
1956 |
(3.235) |
|
jV0jn(eF) |
OOPER |
|||||||
¯ |
|
|
|
This is of course a toy model. The solution including the interaction between all particles – not only between extra ones – has basically the same form except the factor 2 in the enumerator of the exponent is replaced by 1.
This result means that FERMIons with ~p and ~p 0 become correlated, they form a "COOPER-Pair".
The shift in energy can be approximated as
vF p |
, |
|
|
|
|
|
|
|
p |
|
|
(3.236) |
|
|
|
|
|
|
|
vF |
|||||||
If we denote the size of the correlation as x we can approximate |
|
||||||||||||
x |
~ |
|
~ |
vF |
~ eF |
~ |
|
|
|
(3.237) |
|||
|
|
|
|
|
|
|
|
|
|||||
p |
|
pF |
|
pF |
This means the the size of the correlation is much larger than the mean interparticle distance. Therefore a mean field theory can be applied for this system.