“…Indeed, due to the resonant behavior of subwavelength emitters, ,− the absorption cross-section may largely exceed the geometrical cross-section of emitters, ,, resulting in an enhancement of the radiative heat transfer that appears to be super-Planckian. , Nonetheless, if we consider the absorption/emission cross-section as a suitable metric on which the thermal emission power is normalized (as customarily done in antenna theory), such an enhancement vanishes, and even subwavelength emitters are bounded by the usual upper limits imposed by Planck’s radiation law. Moreover, it is worth stressing that, due to the very low emitting power (on the order of nW), the experimental demonstration of super-Planckian emission in subwavelength emitters has turned out to be very challenging, and even though various orders of magnitude of enhancement in far-field radiation with respect to the blackbody spectrum have been claimed, − the highest experimental measurement of emissivity reported so far is still clearly below 1. − Yet, it is possible to overcome Planck’s radiation law just by disregarding each of the underlying constraints, namely, the near-field regime, or the conditions of thermal equilibrium. , In particular, a typical approach to deal with nonequilibrium systems relies on the use of nonlinear media. ,,,, Such is the case, for example, of a semiconductor externally biased either electrically or optically, which produces a redistribution of the energy of electrons and holes in different quasi-Fermi levels described by qV e and qV h , where q and Δ V = V e – V h stand, respectively, for the electron charge and the potential difference. This can be modeled by introducing a nonzero chemical potential, μ F = q Δ V , so that the spectral energy density of nonequilibrium thermal radiation is given by − I NE ( ω , T , μ F ) = ω 2 π 2 c 3 ℏ ...…”