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    Scale-Dependent Heat Transport in Dissipative Media via Electromagnetic Fluctuations

    Matthias Krüger1, Kiryl Asheichyk2, Mehran Kardar3, and Ramin Golestanian4,5

    • 1Institute for Theoretical Physics, University of Göttingen, 37077 Göttingen, Germany
    • 2Department of Theoretical Physics and Astrophysics, Belarusian State University, 5 Babruiskaya Street, 220006 Minsk, Belarus
    • 3Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
    • 4Max Planck Institute for Dynamics and Self-Organization (MPI-DS), D-37077 Göttingen, Germany
    • 5Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford OX1 3PU, United Kingdom

    Phys. Rev. Lett. 132, 106903 – Published 7 March, 2024

    DOI: https://doi.org/10.1103/PhysRevLett.132.106903

    Abstract

    We develop a theory for heat transport via electromagnetic waves inside media, and use it to derive a spatially nonlocal thermal conductivity tensor, in terms of the electromagnetic Green’s function and potential, for any given system. While typically negligible for optically dense bulk media, the electromagnetic component of conductivity can be significant for optically dilute media, and shows regimes of Fourier transport as well as unhindered transport. Moreover, the electromagnetic contribution is relevant even for dense media, when in the presence of interfaces, as exemplified for the in-plane conductivity of a nanosheet, which shows a variety of phenomena, including absence of a Fourier regime.

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