Tunnelling channels form a ring in wavevector space
When the gap is far below the wavelength, all tunnelling wavevectors are much larger than . As in chapter 3, the p reflection coefficient then equals its quasi-static value , independent of , and s polarisation can be neglected.
With , the transmission depends only on and . Near the line, is almost purely imaginary with a large modulus. The transmission is then a function of that reaches exactly 1 at , that is at , and falls off on both sides.
So the tunnelling channels do not fill a disc from zero up to some limit; they sit on a ring of radius about . At too small a wavevector the two surfaces reflect so strongly that energy bounces inside the gap without getting into the other plate; at too large a wavevector the wave decays too fast to get across.
Source: K. Joulain
The number of channels scales as the inverse square of the gap
Change the integration variable from to : . All of moves outside the integral, and what remains depends only on . This step is where the inverse-square law comes from.
The remaining integral has a closed form. Expand the transmission as a geometric series and integrate term by term to get the complex dilogarithm . The course benchmark implements this function independently and compares it with the model’s numerical integral at a 1 nm gap and four frequencies; the largest difference is .
When is close to purely imaginary with a large modulus, the closed form reduces to : the number of channels grows only logarithmically with the strength of the resonance.
The heat transfer coefficient is the ratio of flux to temperature difference as that difference goes to zero. It weights the channel count at each frequency by and integrates. Since the channel count at every frequency scales as , so does the coefficient. Eq. (93) of Joulain et al. states the same conclusion.
Source: K. Joulain
The heat transfer coefficient from the model
The figure shows the heat transfer coefficient between two SiC plates at 300 K against the gap. Above about 10 µm it is nearly constant, about , below the of two black plates for the reason given in chapter 4. Below 1 µm the curve steepens quickly.
A fit between 10 and 50 nm gives an exponent of , close to . The product is , and at 10, 20 and 50 nm. As the gap closes, the share carried by p tunnelling rises from 92% to 99.6% and the curve approaches a pure inverse square.
At 10 nm, : 1530 times two black plates and 2870 times its own value at 100 µm, about three and a half orders of magnitude. Joulain and co-workers write that at 10 nm the coefficient has grown by four orders of magnitude over its far-field value; their Fig. 17 is reproduced from another paper. We did not digitise that figure and have not found the cause of the half-order difference.
The inverse square cannot be pushed to zero gap. Joulain and co-workers mention that it has been questioned because the flux diverges at zero gap; their answer is that the thermal resistance of a 10 nm vacuum gap remains far larger than that of conduction across a hundred nanometres of solid, so the plates can be treated as uniform in temperature. The course model also assumes a local permittivity, so it stops at 10 nm; non-local corrections at smaller gaps were not tested.
Source: K. Joulain · NIST Reference on Constants
Worked example: how many channels open at the line frequency at 10 nm
Problem. Two SiC plates at 300 K are 10 nm apart. At , estimate the number of p tunnelling channels per unit area and compare with two black plates at the same frequency. Then predict the 10 nm coefficient from the 20 nm one.
Model. Use the quasi-static reflection coefficient and the logarithmic approximation, then compare with the closed form.
Numbers. , so , and . The ring radius is . The channel count is ; the closed form gives , or 8690 per square micrometre.
Comparison. Two black plates at this frequency have channels per square micrometre for both polarisations together. Tunnelling opens times more. That many channels exist only in a narrow band around the line, so after integrating over the whole spectrum the coefficient is 1530 times that of black plates.
Prediction. At 20 nm, ; four times that is 9508, while the model gives 9342, so the prediction is 1.8% high. Part of the difference is the 1.5% of the 20 nm flux carried by travelling waves and s tunnelling; the rest is that even the p part is not yet fully quasi-static at 20 nm.
Source: K. Joulain