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D. D. Klug

Publications and source records attributed to D. D. Klug.

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Reply to comment by Witte et al. on "Isochoric, isobaric, and ultrafast conductivities of aluminum, lithium,and carbon in the warm dense matter regime", Phys. Rev. E $96$, 053206 (2017)

In Phys. Rev. E, $99$, 047201 (2019) Witte {\it et al.} have commented on our conductivity calculations [Phys. Rev. E $96$, 053206 (2017)] for warm dense matter (WDM). (i) They criticize our use of the spherically-averaged structure factor $S(k)$ for calculations of the static conductivity $σ$ of FCC aluminum - a common approximation for polycrystalline materials. They themselves give no calculations as their method using density-functional theory (DFT) and molecular dynamics (MD) based Kubo-Greenwood (KG) calculations becomes impractical for cold ions. (ii) We are satisfied that Witte et al. no longer claim a factor of $\sim$ 1.5 change in $σ$ on changing the exchange-correlation (XC) functional used. (iii) They have provided computer-intensive calculations of $σ$ for aluminum using DFT-MD-KG simulations, for temperatures $T$ up to 15 eV but using only $N$=64 atoms in the simulation, where as a mixture of ionic species needs a far larger $N$ to be credible. We present multi-species conductivity calculations via a parameter-free DFT theory [Phys. Rev. E. $52$, 5352 (1995)] for 5 eV to 50 eV. (iv) The conductivities obtained from well-converged DFT-MD-KG methods show a significant underestimate of $σ$; this is especially evident for the isochoric conductivity $σ_{\rm ic}$ extrapolating to $\sim3.5\times 10^6$ S/m, i.e, {\it even below} the experimental {\it isobaric} value of 4.1$\times 10^6$ S/m at the melting point, when a value of $\sim 5\times 10^6$ S/m is anticipated.

cond-mat.stat-mech

Isochoric, isobaric and ultrafast conductivities of aluminum, lithium and carbon in the warm dense matter (WDM) regime

We study the conductivities $σ$ of (i) the equilibrium isochoric state ($σ_{\rm is}$), (ii) the equilibrium isobaric state ($σ_{\rm ib}$), and also the (iii) non-equilibrium ultrafast matter (UFM) state ($σ_{\rm uf}$) with the ion temperature $T_i$ less than the the electron temperature $T_e$. Aluminum, lithium and carbon are considered, being increasingly complex warm dense matter (WDM) systems, with carbon having transient covalent bonds. First-principles calculations, i.e., neutral-pseudoatom (NPA) calculations and density-functional theory (DFT) with molecular-dynamics (MD) simulations, are compared where possible with experimental data to characterize $σ_{\rm ic}, σ_{\rm ib}$ and $σ_{\rm uf}$. The NPA $σ_{\rm ib}$ are closest to the available experimental data when compared to results from DFT+MD, where simulations of about 64-125 atoms are typically used. The published conductivities for Li are reviewed and the value at a temperature of 4.5 eV is examined using supporting X-ray Thomson scattering calculations. A physical picture of the variations of $σ$ with temperature and density applicable to these materials is given. The insensitivity of $σ$ to $T_e$ below 10 eV for carbon, compared to Al and Li, is clarified.

cond-mat.mtrl-sci

A critical assessment of models of pair-interactions and screening used in analyzing recent warm-dense matter (WDM) experiments

Ultra-fast laser experiments yield increasingly reliable data on warm-dense matter (WDM), but rely on entrenched simplistic theoretical models. We re-analyze two topical experiments, avoiding (i) {\it ad hoc} core-repulsion models, (ii) "Yukawa screening" models and (iii) electron-ion equilibrium assumptions. An accurate, rapid density-functional neutral-pseudoatom model coupled to a hyper-netted-chain (HNC) equation with a bridge term is used to compute structure factors, X-Ray scattering, compressibility, phonons and resistivity. Electronic-structure codes are used to confirm the calculations. The Yukawa and core-repulsion models are shown to be misleading.

cond-mat.mtrl-sci

Modelling the atomic structure of very high-density amorphous ice

The structure of very high-density amorphous (VHDA) ice has been modelled by positionally disordering three crystalline phases, namely ice IV, VI and XII. These phases were chosen because only they are stable or metastable in the region of the ice phase diagram where VHDA ice is formed, and their densities are comparable to that of VHDA ice. An excellent fit to the medium range of the experimentally observed pair-correlation function g(r) of VHDA ice was obtained by introducing disorder into the positions of the H2O molecules, as well as small amounts of molecular rotational disorder, disorder in the O--H bond lengths and disorder in the H--O--H bond angles. The low-k behaviour of the experimental structure factor, S(k), is also very well reproduced by this disordered-crystal model. The fraction of each phase present in the best-fit disordered model is very close to that observed in the probable crystallization products of VHDA ice. In particular, only negligible amounts of ice IV are predicted, in accordance with experimental observation.

cond-mat.mtrl-sci