Abstract. Viscous stabilizations of the quantum hydrodynamic equations are studied. The quantum hydrodynamic model consists of the conservation laws for the particle density, momentum, and energy density, including quantum corrections from the Bohm potential. Two different stabilizations are analyzed. First, viscous terms are derived using a Fokker-Planck collision operator in the Wigner equation. The existence of solutions (with strictly positive particle density) to the isothermal, stationary, one-dimensional viscous model for general data and nonhomogeneous boundary conditions is shown. The estimates depend on the viscosity and do not allow to perform the inviscid limit. Second, the numerical viscosity of the second upwind finite-difference discretization of the inviscid quantum hydrodynamic model is computed. Finally, numerical simulations using the non-isothermal, stationary, one-dimensional model of a resonant tunnelling diode show the influence of the viscosity on the solution.Key words. quantum hydrodynamics, viscous quantum hydrodynamics, existence of stationary solutions, numerical dispersion, numerical viscosity, resonant tunnelling diode, semiconductors AMS subject classifications. 76Y05, 35J40, 65N05
IntroductionThe fluiddynamical formulation of the Schrödinger equation, which has been known since the early years of quantum mechanics [32], has been used in many applications for quantum plasmas [34] or quantum semiconductor devices [12,14]. Quantum effects appear through terms involving the Bohm potential and containing third-order derivatives which express the dispersive structure of the equations. These terms are mathematically difficult to handle, and in fact there are only partial analytical and numerical results. This work is devoted to an analytical and numerical study of these equations when they contain additional viscosity terms originating either from particle collisions or from an upwind numerical discretization of the equations.More specifically, we consider the scaled stationary quantum hydrodynamic (QHD) equations for the particle density n, the current density J, and the energy density ne,