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Dresner, Stability of superconductors.2002

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Contents

9.5.

The Kapitza Limit . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . . 180

9.6.

The Two-Dimensional Channel . . . . . . . . . . . . . . . . . . . . . . . .

. . 182

Chapter 10.

Miscellaneous Problems

 

10.1.

An Uncooled Segment of a High-Temperature Superconductor . . 185

10.2.

The Critical Length . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 186

10.3.

Vapor-Cooled Leads . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . .188

10.4.

The Heat BalanceEquation forVapor-Cooled Leads . . . . . . . . .

. . 190

10.5.

Copper Leads . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 191

10.6.

Superconducting Leads . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 193

10.7.

Partly Normal States . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 194

10.8. Partly Normal States: Results and Discussion . . . . . . . . . . . . .

195

Appendix A. The Method of Similarity Solutions

 

A.1.

Partial Differential Equations Invariant to One-Parameter

 

 

Families of One-Parameter Stretching Groups . . . . . . . . . . . .

. . 199

A.2.

Similarity Solutions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 200

A.3.

The Associated Group . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 201

A.4.

Asymptotic Behavior . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 201

A.5. Example: The Superfluid Diffusion Equation . . . . . . . . . . .

. . 202

A.6. Information Obtainable by group Analysis Alone . . . . . . . . .

. . 205

Appendix B.

Stability of the MPZ

 

B.1.

The Ordering Theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 207

B.2.

Proof of the Ordering Theorem . . . . . . . . . . . . . . . . . . . . . . .

. . 207

B.3. Application of the Ordering Theorem to the MPZ . . . . . . . . .

. . 209

B.4.

Lagrangian Formulation and the Stability of Steady States . . . .

. . 209

B.5.

Action Integral of the MPZ . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 211

B.6.

Stability of the Steady States of an Uncooled

 

 

Segment of a Superconductor . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 212

References .

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

. . 215

Index . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .

223

1

Introduction and Overview

1.1. EARLY RESEARCH

The story of superconductivity begins in 1911 with the accidental discovery of superconductivity in mercury by the Dutch physicist Heike Kammerlingh-Onnes. Although the nature of his discovery was not expected, it could have been expected that someone would be doing what he was doing at the time, and it is fair to say that if Kammerlingh-Onnes had not discovered superconductivity when he did, someone else probably would have discovered it during the same epoch of physics.

In 1911, Kammerlingh-Onnes stood at the confluence of several main streams of research in nineteenth-century physics. On the theoretical side, the kinetic theory of gases, Maxwell’s equations of electromagnetism, and Thomson’s discovery of the electron, three of the grand achievements of the century, had been joined by H. Lorentz in his electron theory of metals. On the experimental side, the early attempts of Davy and Faraday to liquefy gases had culminated in Cailletet’s, Pictet’s, and Olszewski-Wroblewski’s liquefaction of oxygen, Dewar’s liquefaction of hydrogen, and Dewar’s invention of the indispensable thermos flask known in scientific circles by his name. So among the attractive possibilities open to physicists at Kammerlingh-Onnes’s time was the study of the properties of metals at low temperatures using liquid cryogens in the hope of better understanding the behavior of the Lorentz electron gas.

Three years earlier, Kammerlingh-Onnes had succeeded in liquefying helium, the last of the so-called permanent gases to be liquefied. With liquid helium in a dewar flask, Kammerlingh-Onnes had a peerless tool for low-temperature research. He picked as his first target the electrical resistance of metals. He had two reasons for his choice (Mendelssohn, 1968). First, Mendelssohn says, Kammerlingh-Onnes felt that the measurement of electrical resistance would be relatively simple and thus a good place to begin. Second, such measurements might help to decide between rival theories then extant of how the electrical resistance of metals behaves

1

2

CHAPTER 1

as the temperature approaches absolute zero. One school of thought held that the electrons would freeze and stop moving, which implied an infinite resistance. Another school, using thermodynamic reasoning based on Nernst’s theorem, argued that the resistance would approach zero smoothly with falling temperature.

As Mendelssohn notes, in 1911 Kammerlingh-Onnes already knew that neither of these ideas applied categorically: early experiments on platinum and gold had showed that at low enough temperatures the resistance approached a finite limit and became independent of temperature. This limit is called the residual resistance and plays an important role in practical matters of magnet design. KammerlinghOnnes rightly attributed the residual resistivity to the scattering of conduction electrons by impurity atoms. What then, he asked, would happen in a very pure material?

Mercury was the clear choice for a test metal because it could easily be purified by multiple distillation. When Kammerlingh-Onnes measured its resistance as a function of temperature, he found that it dropped suddenly at 4.15 K to unmeasurably low values (< 10¯6 of the room temperature value). Such a sudden drop in resistance came as a great surprise, and when it was found to happen also in other metals (e.g., Pb, Sn, In), it inflamed Kammerlingh-Onnes’s mind with visions of resistanceless magnets producing high magnetic fields. Certain difficulties unforeseen (and indeed unforeseeable) dashed these early hopes for high-field magnets, but in the end they were realized, as described below.

In the meanwhile, a question of principle remained: How small was the resistance on the low-temperature side of the discontinuity? Now, measurement alone can never show that a physical quantity is zero, because of the finite precision of our apparatus. Today, based on theories created to explain what we know of superconductivity, we believe the resistance in the superconducting state to be exactly zero. But Kammerlingh-Onnes, with only experiment as his guide, could not be sure.

Accordingly, he set about improving his value of the upper bound to the resistance. He fashioned a loop of superconductor, charged it with current, and monitored the magnetic field outside the dewar flask for any decay. During several hours, he saw none, which bespoke a resistance < 10¯11 of the resistance at room temperature. Mendelssohn (1968) mentions such a persistent-mode experiment of much later vintage that lasted for two years and came to an end only because a transport strike interrupted the supply of liquid helium.

These early researches, which gave birth to the science of superconductivity, were honored in 1913 by the award to Kammerlingh-Onnes of the Nobel Prize in Physics.

Introduction and Overview

3

1.2. CRITICAL TEMPERATURE AND CRITICAL FIELD

The obvious application of superconductivity is to magnets, so it did not take Kammerlingh-Onnes long to discover that the application of too strong a magnetic field destroyed the superconducting state and restored resistivity to the conductor. The level of field at which this happened, only a few hundredths of a tesla, were disappointingly low, and the early vision of high-field superconducting magnets fled. (For comparison, note that the six magnets of the IEA’s Large Coil Task, finished in 1987, weighed approximately 45 tonnes apiece and together produced a field of 9 T, Beard et al., 1988.)

The substance of Kammerlingh-Onnes’s early experimentsis summarized in Fig. 1.1. Here the absolute temperature is the abscissa and the applied magnetic field is the ordinate. At points below and to the left of the curve, the sample is superconducting while at points above and to the right of the curve, the sample is not. Inthe science of superconductivity, the nonsuperconducting, resistive state is called the normal state, by virtue, I suppose, of its having been the earlier state to be recognized.

Thecurve thatseparatesthe normal from the superconductingregionisclosely

approximated bya parabola:

 

B/B c = 1 – (T/T c)2

(1.2.1)

Though accurate enough for the purposes of this monograph, Eq. (1.2.1) is not exact. The intercept on the temperature axis Tc is called the critical temperature;

Figure 1.1. The phase diagram of superconductors as determined in Kammerlingh-Onnes’s early experiments. At points below and to the left of the curve, the sample is superconducting while at points above and to the right of the curve it is not.

CHAPTER 1

Table 1.1. Critical Fields and Temperatures of Some

Superconductors

Superconductor

Critical temperature (K)

Critical field (mT)

In

3.41

28.7

Sn

3.72

30.9

Hg

4.15

41.2

Ta

4.48

82.9

Pb

7.18

80.4

 

 

 

the intercept on the field axis Bc is called the critical field. Table 1.1 gives the critical fields and temperatures of several of the superconductors discovered in the early days of superconductor research.

When a field Bp is applied to the superconductor, it remains superconducting up to some temperature Tp < Tc. The pair of values (Tp, Bp) are the coordinates of some point on the curve separating the superconducting from the normal state. A temperature like Tp lying at an interior point of the curve is often loosely referred to as the critical temperature; a clearer but clumsier nomenclature would be the critical temperature at a field Bp. But in most of the literature, the reader is left to decide from the context what temperature is meant by the designation critical.

After Kammerlingh-Onnes’s initial discoveries, superconductivity research lay fallow for more than two decades owing to the low values of the critical fields noted in Table 1.1. Then Meissner and Ochsenfeld (1933) discovered that superconductors expelled the applied magnetic field from their interiors. They found that if a material was cooled into the superconducting state and then exposed to an external magnetic field, the field would not penetrate the interior of the material until the field reached the critical value (at the particular temperature). Furthermore, they found that if the external field was first applied and then the temperature was decreased, when the temperature dropped below the critical value (at that field), the sample, as it became superconducting, expelled the field from its interior. In short, superconductors are not just perfect conductors, they are also perfect diamagnets. This phenomenon is called the Meissner effect.

1.3 TYPE-II SUPERCONDUCTORS

At first, no one knew that there were two kinds of superconductors. The superconductors discovered by Kammerlingh-Onnes and described above are now known as type-I superconductors or soft superconductors. Today, we know that there is another class of superconductors, known as type-II superconductors or hard superconductors that differ from the type-I superconductors in that they admit the magnetic field into their interiors while still remaining superconducting. It is from

Introduction and Overview

5

Figure 1.2. The phase diagram of type-II superconductors.The lower left-hand region represents a superconducting state exactly like that of type-I superconductors: zero resistance and perfect diamagnetism. The upper right-hand region represents the normal state. The middle region represents the mixed state. The fields Bc1 and B c2 are called the lower and upper critical fields, respectively.

these type-II superconductors that contemporary scientific and commercial superconducting magnets are wound.

Shown in Fig. 1.2 is a phase diagram for the type-II superconductors similar to the phase diagram in Fig. 1.1. But now instead of two regions in the field-tem- perature plane, there are three. The lower left-hand region represents a superconducting state exactly like that of type-I superconductors: zero resistance and perfect diamagnetism. The upper right-hand region represents the normal state. The middle region represents a state, called the mixed state, that requires some detailed description.

The magnetic field that a type-II superconductor admits in the mixed state is not uniform, as classical physics requires, but is confined to discrete bundles called fluxoids (see Fig. 1.3). Each bundle has a normal (i.e., nonsuperconducting) core that is threaded by magnetic field. Outside the core, where the material is superconducting, the magnetic field drops off exponentially. The total magnetic flux

_

15

Wb, where h is Planck’s

associated with one core is f = h/2e = 2.068 x 10¯

 

constant (6.625 x 10¯34 J s) and e is the charge on the electron (1.602 x 10¯19 C). Circling each core in the superconducting region, where the field is falling off, is an electric current, whose strength also falls off exponentially with distance from the core.

The existence of the triangular flux lattice shown in Fig. 1.3 was first proposed on theoretical grounds by Abrikosov (1957). Then Essmann and Träuble (1967) visualized Abrikosov’s flux lattice directly. They exposed the surface of a type-II

6

CHAPTER 1

Figure 1.3. The triangular fluxoid latticeof a type-II superconductor in the mixed state. Each fluxoid has a normal core that is threaded by a quantum of flux. An electric current circles each core in the superconducting region.

superconductor to a puff of cobalt vapor produced by exploding a cobalt wire in the same (cold) chamber as the sample. The cobalt atoms, being ferromagnetic, followed the field lines in their outward flight from the wire and converged on the normal cores where the cores ended on the sample surface, revealing with great clarity the triangular lattice predicted by Abrikosov.

If a current is established in the sample perpendicular to the applied magnetic field (Fig. 1.4), it flows in the superconducting region between the normal cores. This current, called the transport current, by flowing through a region in which there is a magnetic field, feels a sidewise volume force J x B, where J is the transport current density and B is the local field. By the equality of action and reaction, the flux lattice feels a volume force -Jx B. (At this point, it is worth stating explicitly that the flux lattice is not just the triangular array of normal cores, but the entire continuous array of normal cores, circulating currents, and inhomogeneous magnetic field that fills the whole superconductor.) This volume force causes the flux lattice to move as indicated in Fig. 1.4. As fluxoids reach one surface of the sample, they disappear, while new fluxoids appear at the opposite surface, so that a steady flow through the sample is maintained.

If one moves with a velocity v through a region of magnetic field B, one feels an electric field E = v x B. Now the velocity of the transport current relative to the flux lattice, is parallel to J x B, so that in the rest frame of the transport current there is an electric field E that has the direction (J x B) x B. The electric field E thus always has a component in the direction opposite to that of J (see Fig. 1.5). So the

Introduction and Overview

7

Figure 1.4. A sketch showing the volume forces that a transport current and the fluxoid lattice exert on each other.

motion of the flux lattice induces an electric field that opposes the flow of transport current, in short, a back emf.

When an external voltage source, e.g., a battery, is connected across a type-II superconductor, the transport current increases until the back emf just balances the applied voltage. At that point, further increase in the transport current ceases and a steady state prevails. But the battery must be left connected to maintain the transport current and it must supply a steady power J·E d(vol) to overcome the back emf. To the battery, then, the sample shows resistance (called the flux-flow resistance).

Fortunately for the practical applications of type-II superconductors, the flow of the flux lattice is impeded by solid-state defects such as impurities, vacancies, interstitial atoms, dislocations, grain boundaries, and precipitates. If in their motion across the sample, the fluxoids encounter a defect, they are attracted to it.1 If enough such defects are present the entire flux lattice may get snagged on them and be

Figure 1.5. Vector relations among the magnetic field B, the current density J, the velocity v ~ J x B of the transport current relative to the fluxoid lattice , and the electric field E present in the rest frame of the transport current.

8

CHAPTER 1

unable to move. In such a case, the flux-flow resistance vanishes, and the transport current, once established, persists just as in a type-I superconductor.

1.4. PINNING

The immobilizing of the flux lattice by defects and impurities is called pinning. If a transport current (current density J) is flowing in the superconductor and if it is exposed to a magnetic field B transverse to the current (as is typically the case in a conductor in a solenoid), the volumetric Lorentz force JB acting between the current and the fluxoids is restrained by the pinning. But there is a limit to how great a force the pinning centers can sustain, and if the product JB becomes too large, the flux lattice is torn loose and begins to move. Flux-flow resistance appears, and for practical purposes the superconducting ideal of lossless current flow is vitiated.

In a fixed background field B, the largest current density that a type-II superconductor can sustain without the appearance of flux-flow resistance is called the critical current density Jc. The rise in resistivity in a superconductor when the critical current density is surpassed is very rapid, and almost immediately beyond the critical current density, the flux-flow resistivity exceeds by a large margin the residual resistivity of ordinary conductors like copper. So the critical current density can be looked upon as a kind of boundary between two states, one superconducting and the other resistive. In this respect there is a loose analogy between the type-I and type-II superconductors. But it should be emphasized that there is in fact an important difference. When type-I superconductors first become resistive, the superconducting state has been destroyed, but when type-II superconductors first become resistive the superconducting state of quantized fluxoids still persists .

Experiments, among which the earliest were those of Kim, Hempstead, and Strnad (1963), show that the pinning force JcB can be considered independent of B to a rather good approximation. These authors have proposed on the basis of their experiments the empirical formula

Jc = const/(B + Bo)

(1.4.1)

where Bo is a constant of the order of a few hundredths of a tesla. At high fields it can be neglected and the critical current density taken inversely proportional to the field.

Not only does the critical current density Jc decrease with increasing field, but it also decreases with increasing temperature. This is because the pinning energy decreases with increasing temperature (cf. Eq. (2.4.8)). The higher the temperature, therefore, the smaller the Lorentz force JcB required to tear the entire lattice loose and initiate steady flux flow.

Introduction and Overview

9

Even when the pinning force is strong, the flux lattice can creep due to thermal fluctuations. Since the pinning energy is comparable with the thermal energy kT, where k is Boltzmann’s constant and T is the temperature, thermal fluctuations occasionally lift a pinned fluxoid from its pinning site, after which it drifts under the action of the Lorentz force until it encounters another site. Such flux creep is accompanied by the appearance of a small flux-flow resistivity.

Figure 1.6 shows a surface in a three-dimensional space whose axes are temperature T, external magnetic field B, and current density J. Points below the surface correspond to a firmly pinned fluxoid lattice and the absence of resistance to current flow. Points above the surface correspond to flux flow and the presence of resistance. Inside the larger surface, near the origin, is a second much smaller surface that marks the boundary of type-I behavior. At points below that surface, the superconductor exhibits a Meissner effect and is a type-I superconductor. The bounding curve of the smaller surface in the B-T plane is the same as the phase boundary in Fig. 1.2 that separates the Meissner from the mixed state. The current on this lower surface is determined by the Silsbee condition that the sum of the self-field and the background field always be less than the critical field that separates the Meissner from the mixed state (Silsbee, 1916).

On the other hand, the current on the upper surface is determined by the condition that the flux lattice remain pinned, i.e., that there be no flux-flow resistance. The bounding curve of this surface in the B-T plane need not necessarily be the phase boundary in Fig. 1.2 that separates the mixed state from the normal state, and in fact for some of the new high-temperature ceramic superconductors (Tc ~ 100 K ) it is not. For some of those superconductors, there is yet another curve, called the irreversibility curve, that traverses the region of the B-T plane corresponding to the mixed state: on one side of it Jc is finite, on the other Jc = 0. It is the irreversibility curve that determines the practical performance of the high-tem- perature superconductors rather than the phase boundary between the mixed and normal states. On the other hand, for the older, low-temperature superconducting metallic alloys and compounds (e.g., NbTi and Nb3Sn; Tc = 9.6 K and 18 K, respectively), the irreversibility curve and the phase boundary are practically indistinguishable and usually no distinction is made between them. The difference in behavior between the two classes of superconductors is caused, of course, by the quite large difference in the amplitude of the thermal agitation of their fluxoid lattices.

The surface in Fig. 1.6, the so-called critical surface, is the basic datum on which the considerations of this monograph are based. With it in hand we can turn to the stability problem; but first we must begin with a short description of the structure of modern superconducting wires.