2016
DOI: 10.1002/ctpp.201500101
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The Energy‐Autocorrelation Function in Magnetized and Unmagnetized Strongly Coupled Plasmas

Abstract: The 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.

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Cited by 6 publications
(8 citation statements)
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References 50 publications
(42 reference statements)
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“…2 of Ref. [41]). The most notable difference is the absence of persistent oscillations in the pp, vv, and pv terms (labeled pp, cc, and pc in Ref.…”
Section: Simulation Resultsmentioning
confidence: 88%
See 2 more Smart Citations
“…2 of Ref. [41]). The most notable difference is the absence of persistent oscillations in the pp, vv, and pv terms (labeled pp, cc, and pc in Ref.…”
Section: Simulation Resultsmentioning
confidence: 88%
“…2 of Ref. [41] highlights the role of the long range potential in comparison with the shorter-range κ = 2 Yukawa OCP (hereafter YOCP) at values of Γ where liquid like behavior sets in (Γ = 30 − 300 in Fig. 2 of Ref.…”
Section: Simulation Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…The temperature homogenization time scale shows the well-known non-monotonic dependence on the coupling strength Γ which is related to the different modes of thermal diffusion [14,15]. Comparing the isotropization time scale at β = 0 and Γ = 100 (Fig.…”
Section: A Thermal Relaxation Time Scalementioning
confidence: 96%
“…Due to the strong coupling of these dust particles, the collection of dust particles exhibits behaviors of liquids [23,24] and solids [18,25]. Molecular dynamics (MD) simulations of 2D Yukawa liquids and solids have been widely used to study behaviors of 2D dusty plasmas [16,17,[26][27][28][29][30][31][32][33][34][35][36][37].…”
Section: Introductionmentioning
confidence: 99%