Electromagnetism

The force that forgets Planck's constant

Two mirrors in a vacuum attract, with a pressure that contains Planck's constant and nothing else about the world but the speed of light. Warm the mirrors and pull them apart, and past a few micrometres at room temperature the Planck constant drops out of the answer. The force is still there and is now larger than the vacuum alone would give, but it has become classical: a count of thermal fluctuations of the static field, with kT of energy each. Half of that classical force comes from one fluctuation — a static magnetic field — and whether a real metal mirror reflects it is a question that has divided the people who measure the force for twenty years.

Assumes: The attraction that weakens when light is too slow · How many ways there are to vibrate

How many ways there are to vibrate found the Casimir pressure between two mirrors by counting the modes of the field that fit between them. At zero temperature each mode carries its zero-point energy, half of ℏω\hbar\omega; fewer modes fit in the gap than outside it, and the difference in energy pushes the mirrors together with a pressure of π2ℏc/240 a4\pi^2\hbar c/240\,a^4. The attraction that weakens when light is too slow arrived at the same family of forces from two atoms, and found that past a distance set by how fast the source fluctuates, the field’s travel time cuts the slow fluctuations off from the fast ones and the force loses a power of the distance. It ended on a dispute: what happens when the mirrors are not at absolute zero.

The question looks like a matter of small corrections, since room temperature is a modest energy next to the photons that matter at a micrometre. It is not. At a few micrometres the thermal part of the force overtakes the vacuum part. Beyond that it dominates, and it has a remarkable property: Planck’s constant is not in it. The force between two warm mirrors far apart is a classical force, the same one that a nineteenth-century physicist with Maxwell’s equations and Boltzmann’s statistics could have computed. And half of it comes from one particular fluctuation, which a real metal may or may not reflect.

Counting modes at a temperature

The zero-temperature argument puts half a quantum in every mode. At a temperature TT each mode also carries its thermal occupation, ℏω/(eℏω/kT−1)\hbar\omega/(e^{\hbar\omega/kT} - 1), which is large for modes below kT/ℏkT/\hbar and negligible above. The thermal photons push on the mirrors from both sides, and between the plates their spectrum is cut into the same discrete set of modes as the zero-point field. So the warm force is the cold force plus a radiation pressure difference, and the question is how large the difference is.

Lifshitz worked it out in 1956, and the form of his answer is what makes the physics visible. The field’s fluctuations at temperature TT are not summed over all real frequencies but over a comb of imaginary ones, the Matsubara frequencies,

ξn=2πnkTℏ,n=0,1,2,…\xi_n = \frac{2\pi n kT}{\hbar}, \qquad n = 0, 1, 2, \ldots

each contributing a term that dies across the gap as e−2ξna/ce^{-2\xi_n a/c}. That exponential is the retardation of the previous essay in a new costume: a fluctuation at ξn\xi_n cannot correlate the two plates if the light carrying it takes longer than 1/ξn1/\xi_n to cross and return. When the plates are close, the comb’s teeth are so finely spaced compared with the cut-off that the sum is effectively an integral, and the integral is the zero-temperature result. When they are far apart, every term but the static one is cut off, and the force is whatever the static term says.

The spacing of the comb sets the scale. The first nonzero frequency corresponds to a wavelength 2πc/ξ1=ℏc/kT2\pi c/\xi_1 = \hbar c/kT, the thermal length, which at room temperature is 7.63 micrometres. Plates much closer than that see a continuum of fluctuations; plates much farther apart see only n=0n = 0.

Which thermal frequencies carry the force. The share of the Casimir pressure between ideal plates at 300 K carried by each Matsubara frequency ξₙ = 2πnkT/ħ, n = 0 to 11, for separations of 0.5, 2 and 8 μm. ξ₁ corresponds to a wavelength of 7.63 μm. At 0.5 μm the force is spread over many frequencies and the static term n = 0 carries 15.2 per cent: the sum is effectively an integral, which is the zero-temperature limit. At 2 μm it carries 59 per cent; at 8 μm, all but 3.2·10⁻⁴ of it, and the rest is cut off because a fluctuation at ξₙ dies as e^(−2ξₙa/c) across the gap. The n = 0 term is the static, classical fluctuation of the field, with kT of energy per mode; it is the only one whose size does not involve Planck's constant.
Fig. 1 The share of the pressure between ideal plates at 300 K carried by each Matsubara frequency, for three separations. At 0.5 μm the static term n=0n = 0 carries 15 per cent and the rest is spread over many terms; at 2 μm it carries 59 per cent; at 8 μm it carries essentially all of it.

The figure computes the sum for two perfectly reflecting plates at 300 kelvin and shows how the pressure is shared among the terms. At half a micrometre the shares fall off slowly — fifteen per cent from n=0n = 0, twenty-seven from n=1n = 1, and a long tail — which is the signature of a sum behaving like an integral. At two micrometres the static term carries fifty-nine per cent and the next one most of the rest. At eight micrometres the static term carries all but a few parts in a million. There the force is entirely the n=0n = 0 term.

The term with no quantum in it

The n=0n = 0 term is the static limit: fluctuations of the field at zero frequency. In the Matsubara sum it carries a weight of a half, and its size is fixed without any reference to Planck’s constant. For two ideal mirrors it gives

Pcl=ζ(3) kT4πa3,P_{\text{cl}} = \frac{\zeta(3)\,kT}{4\pi a^3},

with ζ(3)=1.202\zeta(3) = 1.202, a pure number. There is kk and TT and the separation, and nothing else. The ħ that sets the Matsubara spacing cancels out of the static term exactly, because a fluctuation at zero frequency has no quantum: a static field mode in thermal equilibrium holds kTkT of energy whatever its frequency, which is equipartition applied to the electromagnetic field. The same counting gives half a kT in a piece of wire, the Johnson noise of a resistor, which contains no ħ either until the frequency rises to kT/ℏkT/\hbar.

So the far-field Casimir force at a temperature is a classical statistical force. The mirrors constrain which static field configurations can exist between them, fewer configurations fit in the gap than outside, and the thermal free energy of the field is lower when the mirrors are close. The pressure is the derivative of that free energy. Its power law, the inverse cube, is one power shallower than the vacuum force’s inverse fourth, because the vacuum force carries an extra factor of ℏc/a\hbar c/a — the energy of a photon whose wavelength fits the gap — where the classical force carries kTkT.

The Casimir pressure between warm plates, from vacuum to heat. The attractive pressure between two parallel, perfectly reflecting plates at 300 K against their separation, on logarithmic axes, from the Lifshitz sum over Matsubara frequencies. Dashed: the zero-temperature law π²ħc/240a⁴. Dotted: the classical law ζ(3)kT/4πa³, which contains no Planck constant. At 1 μm the full pressure is 0.0013 Pa, within 0.2 per cent of the vacuum value; at 10 μm it is 3.96·10⁻⁷ Pa, 3.05 times the vacuum value and within 0.002 per cent of the classical law. The two laws cross at 3.28 μm; the thermal length ħc/kT is 7.63 μm. The second solid curve removes one term — the static magnetic fluctuation, which a metal of finite conductivity does not reflect — and sits 15 per cent lower at 1 μm and a factor of two lower far out. The plates are otherwise ideal mirrors: a model, chosen to isolate that one term.
Fig. 2 The pressure between ideal plates at 300 K (blue) against separation, with the zero-temperature law (dashed) and the classical law (dotted); the green curve drops the static magnetic term. The two laws cross at 3.28 μm.

The figure draws the whole crossover. Below a micrometre the full pressure lies on the zero-temperature line, within two parts in a thousand at 1 μm, where it is 1.3 millipascals. Above ten micrometres it lies on the classical line, and at 10 μm it is 3.05 times what the vacuum alone would give. Between, the curve bends from the inverse fourth power to the inverse third. The two laws are equal at

a∗=π360 ζ(3) ℏckT=0.43 ℏckT,a^* = \frac{\pi^3}{60\,\zeta(3)}\,\frac{\hbar c}{kT} = 0.43\,\frac{\hbar c}{kT},

which is 3.28 micrometres at room temperature. Beyond a∗a^* the plates attract more strongly because they are warm than because they are in a quantum vacuum.

The same crossing at every temperature

Nothing in the argument is special to room temperature. The crossover distance is a fixed multiple of the thermal length, and the thermal length scales as one over the temperature.

The distance beyond which the vacuum force becomes heat. The separation at which the classical, Planck-constant-free part of the Casimir pressure between ideal plates equals the zero-temperature part, a = π³ħc/(60ζ(3)kT), against temperature on logarithmic axes, with the thermal length ħc/kT (dashed). Both fall as one over the temperature; a is 0.43 of the thermal length. Liquid helium, 4.2 K: 234 μm; liquid nitrogen, 77 K: 13 μm; room, 300 K: 3.28 μm; a hot filament, 1000 K: 0.98 μm. Below the line the force is quantum, set by ħ and c alone; above it the force is classical, set by kT, and the plates attract because thermal fluctuations of the static field between them are fewer than outside.
Fig. 3 The separation at which the classical part of the pressure equals the zero-temperature part, against temperature, with the thermal length ℏc/kT\hbar c/kT dashed. Below the line the force is set by ℏc\hbar c; above it, by kTkT.

In liquid helium, at 4.2 kelvin, the crossover is at 234 micrometres, a quarter of a millimetre: anything measured below that is the quantum vacuum force, almost untouched by temperature. In liquid nitrogen it is 13 micrometres. Near a hot filament at a thousand kelvin it is under a micrometre, so the force between two glowing wires a few micrometres apart is classical. The line in the figure divides the plane of temperature and separation into a quantum half, where the force is ℏc/a4\hbar c/a^4 with a small thermal correction, and a classical half, where it is kT/a3kT/a^3 with a small quantum one.

This is the same division that runs through the curve that would not come down, the blackbody problem. There the Rayleigh–Jeans law, classical and correct at long wavelengths, failed at short ones, and Planck’s constant appeared exactly where ℏω\hbar\omega overtook kTkT. Here it is the other way round: the zero-point force, quantum and correct at short distances, fails at long ones, and Planck’s constant disappears exactly where kTkT overtakes ℏc/a\hbar c/a. The crossover is a statement that the gap between the plates is acting as a filter on wavelengths, and the filter’s cut-off is the separation.

How much warmth adds

For ideal mirrors the thermal force only ever adds. That is not what experiment cares about, which is how much it adds at the separations where the force can be measured, and the answer is very little where the measurements are precise.

How much warmth adds to the vacuum force, and how much one term takes away. The Casimir pressure between parallel plates at a temperature, divided by the zero-temperature pressure at the same separation, against separation from 0.1 to 10 μm, at 300 K and 77 K. Upper curves: perfectly reflecting plates. Lower curves: the same plates with the static magnetic fluctuation not reflected, as by a metal of finite conductivity. For ideal plates at 300 K the ratio stays within a per cent of one below about a micrometre and then climbs, reaching 3.05 at 10 μm, because the classical part grows one power of the distance faster than the vacuum part falls. Without the static magnetic term the ratio first falls below one, to 0.659 at 3.16 μm, before warmth wins. At 77 K every feature moves four times further out. The disputed thermal correction is the gap between each pair of curves.
Fig. 4 The pressure at 300 K (solid) and 77 K (dashed) divided by the zero-temperature pressure. Blue: ideal mirrors. Green: the static magnetic term removed, which first pulls the ratio below one, to 0.659 at 3.16 μm at room temperature.

The blue curves divide the warm pressure by the cold one. For ideal plates at room temperature the ratio is within a per cent of one up to about a micrometre and then rises steeply, reaching three at ten micrometres. Cooling to 77 kelvin pushes the rise out by a factor of four. The precision measurements of the Casimir force, which reach the per-cent level, are made between a few hundred nanometres and about a micrometre, because that is where the force is large enough to measure well. The ideal-mirror model says the thermal correction there is a fraction of a per cent, too small to argue about.

The green curves say something else, and they are the subject of the argument.

One fluctuation, and the metal’s choice

A real metal is not an ideal mirror. At high frequencies its electrons cannot follow the field, which reduces the force below a few hundred nanometres; that correction is well understood and is not in dispute. The dispute is at the other end of the comb, at ξ=0\xi = 0, and it concerns one of the two polarisations of the static field.

The n=0n = 0 term has two parts. One is a static electric fluctuation, which any conductor reflects, since a conductor’s charges move to cancel any electric field inside it. The other — called transverse electric, because its electric field lies along the plates — becomes, at zero frequency, a static magnetic field. Whether a metal reflects a static magnetic field depends on what kind of metal it is.

A static magnetic fluctuation, let through or turned away. Two pairs of parallel plates, each crossed by the field lines of a slowly varying magnetic fluctuation. Left: plates of an ordinary metal with finite conductivity. A field that does not change induces no lasting current, so the static field passes straight through the plates, and the gap between them contains the same fluctuation as the space outside: this part of the field exerts no force. Right: plates that reflect perfectly at zero frequency, as the plasma description of a metal assumes and as a superconductor actually does. The static field is excluded from the plates, the gap and the outside hold different fluctuations, and the difference pushes the plates together. That one term — transverse-electric, zero frequency — is half of the classical Casimir force at large separations, and it is the whole of the dispute about how to calculate the force between real metal plates at room temperature.
Fig. 5 A static magnetic fluctuation crossing two pairs of plates. An ordinary metal lets it through (left), so this term exerts no force; a perfect mirror or a superconductor excludes it (right), and the term contributes half of the classical pressure.

An ordinary metal, with finite conductivity, reflects a magnetic field only by the currents the field induces when it changes, as how far a field gets into metal found for the skin depth. A field that does not change induces no lasting current, and it passes through the metal as though it were not there. In that case the static magnetic fluctuation is the same between the plates as outside, and its contribution to the force is zero. Removing it takes away exactly half of the classical term, ζ(3)kT/8πa3\zeta(3)kT/8\pi a^3. This is the Drude description, named after the model of a metal’s electrons as a gas with a collision time, which is the description that fits every optical measurement on metals ever made.

A superconductor behaves the opposite way. It pushes a static magnetic field out, within its penetration depth, and so it reflects the static magnetic fluctuation just as an ideal mirror does. The “plasma” description of a metal — electrons with no collisions at all — does the same, since collisionless electrons screen a static magnetic field the way a superconductor’s pairs do. In that description the static term survives in full.

The two descriptions differ in nothing but how the electrons behave at frequencies below their collision rate, about 101310^{13} per second in gold, and in this one term. At large separations the difference is a factor of two in the force. At a micrometre, in the ideal-mirror model, it is fifteen per cent, and it pulls the green curve in the earlier figure below one: a metal that lets the static magnetic fluctuation through attracts less when warm, by a third at three micrometres, before the remaining classical term takes over further out.

What the measurements have said

The force has been measured with a torsion pendulum, with atomic-force-microscope cantilevers, and with micromechanical oscillators carrying a sphere close to a plate, and the measurements disagree about which description is right in a way that has not resolved.

Precise measurements by Decca and colleagues between about 160 and 750 nanometres, at the per-cent level and below, have repeatedly agreed with the plasma description and disagreed with the Drude description — the one that fits the optical data. A later measurement by the same group, designed to cancel the electrostatic forces from patches of differing surface potential, which are the largest systematic error in every such experiment, gave the same verdict. In 2011 Sushkov, Lamoreaux and colleagues measured at 0.7 to 7 micrometres, where the thermal term is large, and reported a thermal force of the size the Drude description predicts. But to do it they subtracted an electrostatic background many times larger than the thermal force, with a shape fitted to the data, and whether that subtraction leaves the answer they reported or some other one has been argued ever since.

The disagreement has a deeper side. It has been argued that the Drude description, for a metal whose resistance falls to zero at absolute zero as a perfect crystal’s would, gives the Casimir free energy an entropy that does not vanish at zero temperature, in contradiction with the third law. Others have answered that any real crystal has impurities, that their residual resistance restores the third law, and that the contradiction is a property of an idealisation rather than of the Drude description. Neither side has persuaded the other.

Why the static field is the hard part

The difficulty is that the term in question is the one no optical experiment can see directly. A metal’s response is measured with light, at real frequencies, and the response at zero frequency is reached by extrapolation. The Drude model extrapolates through the collision rate to a finite conductivity at zero frequency; the plasma model drops the collisions and extrapolates to an infinite one. At every frequency anyone can shine light at, the two are nearly indistinguishable. At ξ=0\xi = 0 they differ completely, and the static magnetic term sits exactly there.

So the Casimir force at a few micrometres is a measurement of something optics cannot reach: whether a static magnetic fluctuation enters a metal at room temperature. In ordinary physics the answer is not in doubt — a bar magnet’s field passes straight through a copper sheet — but the thermal fluctuations of the field are not a bar magnet, and the question is whether the Lifshitz formula, with the measured conductivity put into it, is the right description of how a metal’s electrons respond to fluctuations at all. It may be that the formula needs a correction for how electrons near the surface behave that neither model contains, and several have been proposed. None has yet been confirmed.

A proposed way out uses superconductors. Cooling a metal film through its superconducting transition switches its response to the static magnetic field from transmitting to excluding, while changing its optical response hardly at all, so the change in the Casimir energy across the transition would isolate exactly the term in dispute. The change is tiny and the measurement is extremely hard, and it has been proposed rather than completed.

A classical force hidden inside a quantum one

The surprising thing is where the classical force has been hiding. The Casimir effect is introduced, rightly, as the cleanest mechanical evidence of the zero-point energy of the field, and at the separations where it was first measured convincingly — a fraction of a micrometre — it is exactly that. Yet the same calculation, carried a few micrometres further at room temperature, delivers a force that Maxwell and Boltzmann could have computed, larger than the quantum one, and independent of Planck’s constant.

The two forces are the two ends of one sum. The zero-point force is what the sum gives when the teeth of the Matsubara comb are dense; the classical force is its static term alone. Which one a measurement sees depends on a single ratio, the separation against ℏc/kT\hbar c/kT. The same ratio decides when a blackbody’s spectrum is classical, when a resistor’s noise is classical and when the heat crossing a gap too narrow for light is set by evanescent waves rather than by photons that travel, and the near-field heat flow and the thermal Casimir force are, in Lifshitz’s formulation, two outputs of one calculation.

What the pictures cannot show

The figures use plates that reflect perfectly at every nonzero Matsubara frequency, to isolate the one term in dispute. A real gold plate reflects less well above its plasma frequency, which lowers the force below a few hundred nanometres by ten per cent and more, and has its own small temperature dependence; the figures leave both out. They are drawn for parallel plates, while almost every experiment uses a sphere near a plate, related to the plates by an approximation that is good to a fraction of a per cent at the distances used. And they show no electrostatic patch forces, roughness or residual gas, which in practice are larger than the thermal effect wherever it is large, and which are why its measurement is still argued over.

Still open: what a metal does with a static fluctuation

The question has narrowed to one number: the reflection coefficient of a metal at zero frequency for the transverse electric polarisation, which the Drude description sets to zero and the plasma description to one. Optical data cannot decide it, and the force measurements that can have disagreed. What would settle it is a measurement of the thermal force at several micrometres with the electrostatic background controlled independently rather than fitted, or a measurement across a superconducting transition, or a theory of the electrons at a metal’s surface that predicts which description applies before it is measured. None exists yet.

The habit worth carrying away is to ask which term of a sum survives in a limit, and what it contains. A sum over the frequencies of a field’s fluctuations becomes, at large separation, its zero-frequency term alone, and that term carries kT per mode and no Planck constant — so the force between warm mirrors far apart is classical, with a crossover at 0.43 ħc/kT, 3.3 μm at room temperature. Half of that classical force is a static magnetic fluctuation, and whether a metal mirror reflects it is the one thing about the Casimir force that is still not known.

Part 6 of 6

This essay is one argument about Retardation. The others:

The objects named here

The third axis, after the field and the reading path: the things themselves, and every essay that touches each one.

Casimir effectClassical limitEquipartitionFluctuationsMatsubara frequencySuperconductivityThermal wavelengthZero-point energy