“…The near-field radiation between the emitter and the PV cell is calculated by adding contributions of propagating and evanescent modes, as ,, where Θ(ω, T i ) = ℏω/{exp[ℏω/( k B T i )] – 1} is the mean energy of the Planck oscillator, ω is the angular frequency, ℏ is the reduced Planck constant, k B is the Boltzmann constant, and T 1 and T 2 are the temperature of the emitter and the PV cell, respectively. The exchange functions for propagating and evanescent waves are expressed by where r 01 p,s and r 02 p,s are the modified reflection coefficients for the vacuum/doped-Si/SiO 2 (or vacuum/SiO 2 ) and vacuum/Au/ n -GaSb multilayers, respectively.…”