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Patterson, Bailey - Solid State Physics Introduction to theory

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8.3 Tunneling (B, EE) 477

We seek solutions of the form (any complex function can always be written as a product of amplitude ρ and eiφ where φ is the phase)

ψ1 = ρ1 exp(iϕ1) ,

 

(8.60)

ψ2 = ρ2 exp(iϕ2 ) .

 

(8.61)

So, using (8.58) and (8.59) we get

 

 

iρ1 ρ1ϕ1 =Uρ2 exp(i

ϕ) ,

(8.62)

iρ2 ρ2ϕ2 =Uρ1 exp(i

ϕ) ,

(8.63)

where

 

 

ϕ = (ϕ2 ϕ1)

 

(8.64)

is the phase difference between the electrons on the two sides. Separating real and imaginary parts,

ρ1 =Uρ2 sin ϕ ,

(8.65)

ρ1ϕ1 = −Uρ2 cos

ϕ ,

(8.66)

ρ2 = −Uρ1 sin

ϕ ,

(8.67)

ρ2ϕ2 = −Uρ1 cos

ϕ .

(8.68)

Assume ρ1 ρ2 ρ for identical superconductors, then

 

 

d

 

(ϕ

2

ϕ ) = 0 ,

(8.69)

 

 

 

dt

1

 

 

 

 

 

 

 

ϕ2 ϕ1 constant ,

(8.70)

 

 

 

ρ1 ρ2 .

 

(8.71)

The current density J can be written as

 

 

 

J

d

ρ22 = 2ρ2ρ2 ,

(8.72)

dt

 

 

 

 

 

 

 

so

 

 

 

 

J = J0 sin(ϕ2 ϕ1) .

(8.73)

This predicts a dc current with no applied voltage. This is the dc Josephson effect. Another more rigorous derivation of (8.73) is given in Kuper [8.20 p 141]. J0 is the critical current density or the maximum J that can be carried by Cooper pairs.

478 8 Superconductivity

The ac Josephson effect occurs if we apply a voltage difference V across the junction, so that qV with q = 2e is the energy change across the junction. The relevant equations become

i

∂ψ1

=

Uψ2 eV ψ1 ,

(8.74)

t

 

 

 

 

 

 

i

∂ψ2

 

=

Uψ1 + eV ψ2 .

(8.75)

 

 

 

t

 

 

 

 

 

Again,

 

 

 

 

 

 

iρ1 ρ1ϕ1 =Uρ2 exp(i

ϕ) eVρ1 ,

(8.76)

iρ2 ρ2ϕ2 =Uρ1 exp(i ϕ) + eVρ2 .

(8.77)

So, separating real and imaginary parts

 

 

 

 

ρ1 =Uρ2 sin

ϕ

(8.78)

 

ρ2 = −Uρ1 sin

ϕ

(8.79)

 

 

 

ρ1 ρ2

 

(8.80)

ρ1ϕ1 = −Uρ2 cos

ϕ + eV

(8.81)

ρ2ϕ2 = −Uρ1 cos

ϕ eV .

(8.82)

Remembering ρ1 ρ2 ρ, so

 

 

 

 

 

 

 

ϕ2 ϕ1 2eV .

(8.83)

Therefore

 

 

 

 

 

 

 

ϕ (

ϕ)0 2eVt ,

(8.84)

and

 

 

 

 

 

 

J = J0 sin[( ϕ)0 2eVt] .

(8.85)

Again, J0 is the maximum current carried by Cooper pairs. Additional current is carried by single-particle excitations producing the voltage V. The idea is shown later in Fig. 8.18. Therefore, since V is voltage in units of , the current oscillates with frequency (see (8.85))

ωJ = 2eV = 2e

Voltage

.

(8.86)

 

For the dc Josephson effect one can say that for low enough currents there is a current across the insulator in the absence of applied voltage. In effect because of the coherence of Cooper pairs, the insulator becomes a superconductor. Above a critical voltage, Vc, one has single electrons and the material becomes ohmic rather than superconducting. The junction then has resistance, but the current also has a component that oscillates with frequency ωJ as above. One understands this by saying that above Vc one has single particles as well as Cooper pairs. The

8.4 SQUID: Superconducting Quantum Interference (EE) 479

Cooper pairs change their energy by 2eV = ωJ as they cross the energy gap causing radiation at this frequency. The ac Josephson effect, which occurs when

ω =

q

Voltage

(8.87)

 

is satisfied, is even more interesting. With q = 2e (for a Cooper pair), (8.87) is believed to be exact. Thus, the ac Josephson effect can be used for a precise determination of e/ . Parker, Taylor, and Langenberg6 have done this. They used their new value of e/ to determine a new and better value of the fine structure constant α. Their new value of α removed a discrepancy between the quantumelectrodynamics calculation and the experimental value of the hyperfine splitting of atomic hydrogen in the ground state. These experiments have also contributed to better accuracy in the determination of the fundamental constants. There have been many other important developments connected with the Josephson effects, but they will not be presented here. Reference [8.20] is a good source for further discussion. See also Fig. 8.18 for a summary.

Finally, it is worth pointing out another reason why the Josephson effects are so interesting. They represent a quantum effect operating on a macroscopic scale. We can play with words a little, and perhaps convince ourselves that we understand this statement. In order to see quantum effects on a macroscopic scale, we must have many particles in the same state. For example, photons are bosons, and so, we can obtain a large number of them in the same state (which is necessary to see the quantum effects of electrons on a large scale). Electrons are fermions and must obey the Pauli principle. It would appear, then, to be impossible to see the quantum effects of electrons on a macroscopic scale. However, in a certain sense, the Cooper pairs having total spin zero, do act like bosons (but not entirely; the Cooper pairs overlap so much that their motion is highly correlated, and this causes their motion to be different from bosons interacting by a two-boson potential). Hence, we can obtain many electrons in the same state, and we can see the quantum effects of superconductivity on a macroscopic scale.

8.4 SQUID: Superconducting Quantum Interference (EE)

A Josephson junction is shown in Fig. 8.17 below. It is basically a superconduc- tor–insulator–superconductor or a superconducting “sandwich”. We now show how flux, due to B, threading the circuit can have profound effects. Using (8.4) with φ the Ginzburg–Landau phase, we have

J = nq

 

ϕ

q

A .

(8.88)

c

m

 

 

 

 

6 See [8.24].

480 8 Superconductivity

Integrating along the upper path gives

 

 

 

 

 

 

 

 

 

 

 

 

 

ϕ1

= β

m

J dl1 +

q

 

β A dl1 ,

(8.89)

 

 

 

 

 

 

α nq

 

 

 

 

 

c α

 

 

 

while integrating along the lower path gives

 

 

 

 

 

 

 

 

 

ϕ2

= β

m

J dl2 +

 

q

β A dl2 .

(8.90)

 

 

 

 

 

α nq

 

 

 

 

 

c α

 

 

 

Subtracting, we have

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

( ϕ1

ϕ2 ) =

m J dl + q

A dl ,

(8.91)

 

 

 

 

 

 

nq

 

 

 

c

 

 

 

 

 

S

 

 

 

 

 

 

 

 

 

 

S

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(1)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

I

 

 

 

 

 

 

 

 

α

 

×

 

 

 

 

 

×

 

β

 

 

 

 

 

B

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

I

(2)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

S

S

Fig. 8.17. A Josephson junction

Fig. 8.18. Schematic of current density across junction versus V. The Josephson current 0 < J < J0 occurs with no voltage. When J > J0 at Vc Eg/e, where Eg is the energy gap, one also has single-particle current

8.4 SQUID: Superconducting Quantum Interference (EE) 481

where the first term on the right is zero or negligible. So, using Stokes Theorem and B = × A (and choosing a path where J 0)

ϕ1

ϕ2 =

q

A dl =

 

q

 

B dA = qΦ

.

(8.92)

 

 

c

 

 

 

 

 

 

 

 

c

 

 

 

 

 

 

 

 

 

 

 

c

 

 

Defining Φ0 = c/q as per (8.45), we have

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

ϕ ϕ

 

 

=

Φ

,

 

 

 

 

 

 

 

 

(8.93)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

2

 

 

Φ0

 

 

 

 

 

 

 

 

 

so when Φ = 0, and φ1 =

φ2. We assume the junctions are identical so defining

φ0 = ( φ1 + φ2)/2, then

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

ϕ = ϕ

0

+

 

 

Φ

 

 

 

,

 

 

 

 

 

 

 

 

(8.94)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

2Φ0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

ϕ2

= ϕ0

 

 

Φ

 

 

 

 

 

 

 

 

 

 

 

 

 

(8.95)

 

 

 

2Φ0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

is a solution. By (8.73)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

JT = J1 + J2 = J0 (sin

 

 

ϕ1 + sin

ϕ2 )

 

 

 

 

 

 

ϕ

+ ϕ

2

 

 

 

 

 

ϕ

ϕ

2

(8.96)

= 2J0 sin

 

1

2

 

 

 

cos

1

2

 

.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

So

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

JT = 2J0 sin(ϕ0 ) cos

 

Φ

 

,

 

 

 

(8.97)

 

2Φ0

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

and

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Φ

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

JT

 

=

2J0

 

 

 

 

 

 

 

 

.

 

 

 

 

(8.98)

 

 

cos

 

 

 

 

 

 

 

 

 

 

 

 

 

max

 

 

 

 

 

 

 

2Φ0

 

 

 

 

 

 

 

 

The maximum occurs when Φ = 2nπΦ0. Thus, quantum interference can be used to measure small magnetic field changes. The maximum current is a periodic function of Φ and, hence, measures changes in the field. Sensitive magnetometers have been constructed in this way. See the original paper about SQUIDS by Silver and Zimmerman [8.31].

8.4.1 Questions and Answers (B)

Q1. What is the simplest way to understand the dc Josephson effect (a current with no voltage in a super–insulator–super sandwich or SIS)?

482 8 Superconductivity

A. If the insulator is much thinner than the coherence length, the superconducting pairs of electrons tunnel right through, and the insulator does not interfere with them–it is just one superconductor.

Q2. What is the simplest way to understand the ac Josephson effect (a current with a component of frequency 2eV/ , where V is the applied voltage)?

A. The Cooper pairs have charge q = 2e, and when they tunnel across the insulator, they drop in energy by qV. Thus they radiate with frequency qV/ . This radiation is linked to the ac current.

8.5 The Theory of Superconductivity 7 (A)

8.5.1Assumed Second Quantized Hamiltonian for Electrons and Phonons in Interaction (A)

As has already been mentioned, in many materials the superconducting state can be accounted for by an attractive electron–electron interaction due to the virtual exchange of phonons. See, e.g., Fig. 8.19. Thus, if we are going to try to understand the theory of superconductivity from a microscopic viewpoint, then we must examine, in detail, the nature of the electron–phonon interaction. There is no completely rigorous road to the BCS Hamiltonian. The arguments given below are intended to show how the physical origins of the BCS Hamiltonian could arise. It is not claimed that this is the way it must arise. However, given the BCS Hamiltonian, it is fair to say that the way it describes superconductivity is well understood.

One could draw an analogy to the Heisenberg Hamiltonian. The road to this Hamiltonian is also not rigorous for real materials, but there seems to be no doubt that it well describes magnetic phenomena in at least certain materials. The phenomena of superconductivity and ferromagnetism are exact, but the road to a quantitative description is not.

We thus start out with the Hamiltonian, which represents the interaction of electrons and phonons. As before, an intuitive approach suggests

H ep = xlb [ xlbU (ri )]x=0 .

(8.99)

l,b

 

We have already discussed this Hamiltonian in Chap. 4, which the reader should refer to, if needed. By the theory of lattice vibrations, we also know that (see Chaps. 2 and 4)

xl,b = −

2Nm ω

[exp(iq l)eq*,b, p (aq, p aq, p )] .

(8.100)

q, p

b

q, p

 

7 See Bardeen et al [8.6].

8.5 The Theory of Superconductivity (A)

483

 

 

In the above equation, the a are, of course, phonon creation and annihilation operators.

By a second quantization representation of the terms involving electron coordinates (see Appendix G), we can write

U (ri ) = ψk xl,bU (ri ) ψkCkCk,

(8.101)

xl,b k,k

 

where the C are electron creation and annihilation operators. The only quantities that we will want to calculate involve matrix elements of the operator Hep. As we have already shown, these matrix elements will vanish unless the selection rule q = kk Gn is obeyed. Neglecting umklapp processes (assuming Gn = 0 the first major approximation), we can write

H ep = −i∑ ∑ ∑

2Nm ω

q, p

exp(iq l)

 

 

 

 

 

 

 

 

 

 

(8.102)

l,b q, p k,k

 

 

 

b

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

× ψ

e*

 

 

xlb

U (r ) ψ

k

δ k′−k (a

a

q, p

)CC

k

,

 

k q,b, p

 

 

 

 

i

 

q

 

q, p

 

 

k

 

 

or

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

H ep = −i∑ ∑ ∑

2Nm ω

q, p

exp(iq l)

 

 

 

 

 

 

 

 

 

 

(8.103)

l,b q, p k,k

 

 

 

b

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

× ψ

 

e*

 

p

 

xlb

U (r ) ψ

k

(a

a

q, p

)C

′−q

C

k

.

 

k′−q q,b,

 

 

i

 

q, p

 

k

 

 

 

Making the dummy variable changes kk, q → −q, and dropping the sum over p (assuming, for example, that only longitudinal acoustic phonons are effective in the interaction—this is the second major approximation), we find

 

H ep = i BqCk

+qCk (aq aq )

(8.104)

 

k,q

 

 

where

 

 

 

Bq =

exp(iq l) ψk +q e*q,b xl,bU (ri ) ψk .

(8.105)

l,b

2Nmbωq

 

 

The only property of Bq that we will use from the above equation is Bq = Bq*. From any reasonable, practical viewpoint, it would be impossible to evaluate the above equation directly and obtain Bq. Thus, Bq will be treated as a parameter to be evaluated from experiment. Note that so far we have not made any approximations that are specifically restricted to superconductivity. The same Hamiltonian could be used in certain electrical-resistivity calculations.

484 8 Superconductivity

We can now write the total Hamiltonian for interacting electrons and phonons (with = 1, and neglecting the zero-point energy of the lattice vibrations):

H = H 0 + H ep = ωqaqaq + εkCkCk + i BqCk

+qCk (aq aq ) , (8.106)

q

k

q,k

 

where the first two terms are the unperturbed Hamiltonian H0.

The first term is the Hamiltonian for phonons only (with nq = aqaq as the phonon occupation number operator). The second term is the Hamiltonian for electrons only (with nk = CkCk as the electron occupation number operator). The third term represents the interaction of phonons and electrons. We have in mind that the second term really deals with quasielectrons. We can assign an effective mass to the quasielectrons in such a manner as partially to take into account the electron– electron interactions, electron interactions with the lattice, and at least partially any other interactions that may be important but only lead to a “renormalization” of the electron mass. Compare Sects. 3.1.4, 3.2.2, and 4.3, as well as the introduction in Chap. 4. We should also include a screened Coulomb repulsion between electrons (see Sect. 9.5.3), but we neglect this here (or better, absorb it in Vk,k—to be defined later).

Various experiments and calculations indicate that the energy per atom between the normal and superconducting states is of order 10−7 eV. This energy is very small compared to the accuracy with which we can hope to calculate the absolute energy. Thus, a frontal attack is doomed to failure. So, we will concentrate on those terms leading to the energy difference. The rest of the terms can then be pushed aside. The results are nonrigorous, and their main justification is the agreement we get with experiment. The method for separating the important terms is by no means obvious. It took many years to find. All that will be done here is to present a technique for doing the separation.

The technique for separating out the important terms involves making a canonical transformation to eliminate off-diagonal terms of O(Bq) in the Hamiltonian. Before doing this, however, it is convenient to prove several useful results. First, we derive an expansion for

 

 

 

 

H S (eS )(H )(eS ) ,

 

 

 

 

 

 

 

 

(8.107)

where S is an operator.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(e

S

)(H )(e

S

 

S +

1

S

2

 

 

 

 

+ S +

1

S

2

 

 

 

 

 

) = 1

2

 

+... H 1

2

 

+...

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(8.108)

 

 

 

 

= H SH + HS +

1 S 2H SHS +

1

HS 2 ,

 

 

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

2

 

 

 

but

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

[[H , S], S] =

[HS SH , S]

=

 

1

HS

2

+

1

S

2

 

 

 

 

,

(8.109)

2

 

2

 

H SHS

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

8.5 The Theory of Superconductivity

(A) 485

 

 

 

 

 

so that

 

 

 

 

H S

= H +[H , S] +

1

[[H ,S],S] +….

(8.110)

 

 

2

 

 

We can treat the next few terms in a similar way.

The second useful result is obtained by H = H0 + XHep where X is eventually going to be set to one. In addition, we choose S so that

ΧH ep +[H 0 , S] = 0 .

(8.111)

We show that in this case HS has no terms of O(X). The result is proved by using (8.110) and substituting H = H0 + XHep. Then

H S = H 0 + ΧH ep + [ H 0 + ΧH ep

,S ] +

1

[[ H 0 + ΧH ep ,S ],S ] +…

 

 

 

 

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

= H 0 + X H ep + [ H 0 ,S ] + X [ H ep ,S ]

 

 

 

(8.112)

 

1

 

 

X

 

 

 

 

 

 

 

 

+

 

[[ H 0 ,S ],S ] +

 

[[ H ep ,S ],S ] +….

 

 

 

 

2

2

 

 

 

 

Using (8.111), we obtain

 

 

 

 

 

 

 

 

H S

= H 0

+ X[H ep ,S] +

X

[[H ep , S],S] + 1 [[H

0 , S],S] +… .

(8.113)

 

 

 

 

 

2

 

 

2

 

 

 

 

Since

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

ΧH ep +[H 0 , S] = 0 ,

 

 

 

(8.114)

we have

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Χ [H ep , S] = −[[H 0 , S], S] ,

 

 

 

(8.115)

so that

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

H S = H 0 + Χ [H ep , S] +

Χ

[[H ep , S], S]

Χ

 

[H ep , S] ,

(8.116)

 

 

 

 

 

 

 

 

 

2

 

 

 

2

 

 

or

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

H S = H 0 +

X

[H ep , S] + O(X 3) .

 

 

(8.117)

 

 

 

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

Since O(S) = X the second term is of order X2, which was to be proved.

The point of this transformation is to push aside terms responsible for ordinary electrical resistivity (third major transformation). In the original Hamiltonian, terms in X contribute to ordinary electrical resistivity in first order.

486 8 Superconductivity

From XHep + [H0,S] = 0, we can calculate S. This is especially easy if we use a representation in which H0 is diagonal. In such a representation

n XH ep m + n H 0S SH 0 m = 0 ,

(8.118)

or

 

 

n XH ep m + (En Em ) n S m = 0 ,

(8.119)

or

 

 

n S m =

n XH ep m

 

Em En .

(8.120)

The above equation determines the matrix elements of S and, hence, defines the operator S (for Em En).

8.5.2Elimination of Phonon Variables and Separation of Electron– Electron Attraction Term Due to Virtual Exchange of Phonons

(A)

Let us now connect the results we have just derived with the problem of superconductivity. Let XHep be the interaction Hamiltonian for the electron–phonon system. Any operator that we present for S that satisfies

n S m =

n ΧH ep m

(8.121)

Em En

is good enough. In the above equation, |m means both electron and phonon states. However, let us take matrix elements with respect to phonon states only and select S so that if we were to take electronic matrix elements, the above equation would be satisfied. This procedure is done because the behavior of phonons, except insofar as it affects the electrons, is of no interest. The point of this Section is then to find an effective Hamiltonian for the electrons.

We begin with these ideas. Taking phonon matrix elements, we have

nq+1 S nq

=

 

 

nq+1 ΧH ep nq

 

 

 

 

E(total initial state)E(total final state)

 

 

 

 

 

= i Bq

Ck+qCk nq+1 aq aq nq

 

 

 

 

Eq+ εk

(Eq+ωq) εk +q

 

 

 

 

 

k,q

 

 

(8.122)

 

 

 

 

C

C

 

n

+1 a

n

 

 

 

 

 

 

k

 

 

 

 

= −i Bq

k +q

 

q

q

q

,

 

 

 

Eq(Eq

+ωq) +εk

εk +q

 

 

 

 

k,q

 

 

 

 

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