Abstract
AbstractThe energy‐autocorrelation function is calculated for a screened Coulomb system in equilibrium and the contributions of different energy transport channels to the total heat conductivity are explored for magnetized and unmagnetized systems. A special focus is on the time scales of the energy‐autocorrelation function which contribute to the field‐parallel enhancement of heat conduction in strongly coupled plasmas. The investigation is based on first‐principle molecular dynamics simulations. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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