Super-Planckian Electron Cooling in a van der Waals Stack
Radiative heat transfer (RHT) between macroscopic bodies at separations that are much smaller than the thermal wavelength is ruled by evanescent electromagnetic modes and can be orders of magnitude more efficient than its far-field counterpart, which is described by the Stefan-Boltzmann law. In this...
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Veröffentlicht in: | Physical review letters 2017-03, Vol.118 (12), p.126804-126804, Article 126804 |
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Sprache: | eng |
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