Abstract
A semiconductor Boltzmann equation with a non-linear BGK-type collision operator is analyzed for a cloud of ultracold atoms in an optical lattice: \begin{document} $ \partial _t f + \nabla _pe(p)·\nabla _x f - \nabla _x n_f·\nabla _p f = n_f(1- n_f)(\mathcal{F}_f-f),\;\;\;\; x∈\mathbb{R}^d, p∈\mathbb{T}^d, t>0. $ \end{document} This system contains an interaction potential \begin{document}$n_f(x,t): = ∈t_{\mathbb{T}^d}f(x,p,t)dp$\end{document} being significantly more singular than the Coulomb potential, which is used in the Vlasov-Poisson system. This causes major structural difficulties in the analysis. Furthermore, \begin{document}$e(p) = -\sum_{i = 1}^d$\end{document} \begin{document}$\cos(2π p_i)$\end{document} is the dispersion relation and \begin{document}$\mathcal{F}_f$\end{document} denotes the Fermi-Dirac equilibrium distribution, which depends non-linearly on \begin{document}$f$\end{document} in this context. In a dilute plasma—without collisions (r.h.s \begin{document}$. = 0$\end{document} )—this system is closely related to the Vlasov-Dirac-Benney equation. It is shown for analytic initial data that the semiconductor Boltzmann equation possesses a local, analytic solution. Here, we exploit the techniques of Mouhout and Villani by using Gevrey-type norms which vary over time. In addition, it is proved that this equation is locally ill-posed in Sobolev spaces close to some Fermi-Dirac equilibrium distribution functions.
Highlights
The theory of charge transport in semiconductors has become a thriving field in applied mathematics
The description of charge transport in semiconductors was extended by an experimental model [21]: a cloud of ultracold atoms in an optical lattice
The ultracold atoms stand for the charged electrons and the optical lattice describes the periodic potential of the crystal, formed by the ions of the semiconductor
Summary
The theory of charge transport in semiconductors has become a thriving field in applied mathematics. By taking the quasineutral limit, they prove the existence of a unique local solution f ∈ C([0, T ], H2m−1,2r(R3× T3)) of the Vlasov-Dirac-Benney equation. They require that the initial data f0 ∈ H2m,2r(R3 × T3) satisfies the Penrose stability condition inf inf 1−. In a realistic physical experiment, the most part of the particle cloud is localized at the origin meaning that the density distribution tends to zero as |x| → ∞ These functions have to be treated with caution since the Fermi-Dirac distributions Ff are not analytic in f = 0 as we can see in the following remark.
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