The pair-interactions U_{ij}® determine the thermodynamics and linear
transport properties of matter via the pair-distribution functions (PDFs),
i.e., g_{ij}®. Great simplicity is achieved if U_{ij}® could be directly
used to predict material properties via classical simulations, avoiding
many-body wavefunctions. Warm dense matter (WDM) is encountered in
quasi-equilibria where the electron temperature differs from the ion
temperature T_i, as in laser-heated or in shock-compressed matter. The electron
PDFs g_{ee}® as perturbed by the ions are used to evaluate fully non-local
exchange-correlation corrections to the free energy, using Hydrogen as an
example. Electron-ion potentials for ions with a bound core are discussed with
Al and Si as examples, for WDM with T_e \ne T_i, and valid for times shorter
than the electron-ion relaxation time. In some cases the potentials develop
attractive regions, and then become repulsive and Yukawa-like' for higher $T_e$. These results clarify the origin of initial phonon-hardening and rapid release. Pair-potentials for shock-heated WDM show that phonon hardening would not occur in most such systems. Defining meaningful quasi-equilibrium static transport coefficients consistent with the dynamic values is addressed. There seems to be no meaningful static conductivity’ obtainable by extrapolating
experimental or theoretical \sigma(\omega, T_i, T_e) to \omega \to 0, unless
T_i \to T_e as well. Illustrative calculations of quasi-static resistivities
R(T_i,T_e) of laser-heated as well as shock-heated Aluminum and Silicon are
presented using our pseudopotentials, pair-potentials and classical integral
equations. The quasi-static resistivities display clear differences in their
temperature evolutions, but are not the strict \omega \to 0 limits of the
dynamic values.

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