One of the hidden heroes of the modern world is heat transfer. Sucking the heat out of modern electronics is a technical feat all by itself. And we’ve tackled even stickier situations, like cooling objects in the vacuum of space.
Heat transfer is governed by laws that have been tested for over a century. These elderly laws are mostly undefeated and undefeatable. But there are a few exceptions. And researchers have now found another exception: beating the limits of radiative heat transfer.
So hot it glows
In electronics, heat can be conducted away to large surfaces, where convection can take care of the rest. In space, there is no convection; everything has to be radiated. The nice feature about radiative heat transfer (often referred to as “blackbody radiation”) is that it is radiative. Heating and cooling can take place over long distances—light from the Sun warms the Earth through radiative heat transfer.
A less nice feature of radiative transfer is its efficiency. The temperature difference between the heat source and the heat sink has to be quite large before any reasonable amount of energy is transferred. In most cases, radiative heat transfer is negligible, but as soon as the temperature goes up substantially, it dominates conduction and convection.
Two of the assumptions used to obtain the rules of blackbody radiation provide loopholes. It was assumed that the radiating and absorbing body were far away from each other compared to the wavelength of the light transferring the heat and that the source and sink were also large compared to the wavelength.
Hey, Tiny, are you packing heat?
A more detailed exploration showed that if either of these two conditions were violated, radiative heat transfer could be made more efficient. In particular, the new theory predicted that there might not even be a limit for heat transfer from objects that were physically smaller than the wavelength of light they radiate. That seems pretty cool (or hot, depending on the perspective).
Previous work had shown that if the source and sink were close to each other, radiative heat transfer could significantly exceed the limits of blackbody radiation. However, all experiments on small emitters and receivers had failed to do so. In the latest installment of the story, researchers have finally shown that the blackbody law can be beaten for objects that are far enough apart.

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