Durand, M.Schuck, PeterViñas Gausí, Xavier2009-09-252009-09-2519871050-2947https://hdl.handle.net/2445/9439The phase-space distribution of semi-infinite nuclear matter is expanded in an ħ series analogous to the low-temperature expansion of the Fermi function. Besides the usual Wigner-Kirkwood expansion, oscillatory terms are derived. In the case of a Woods-Saxon potential, a smallness parameter is defined, which determines the convergence of the series and explains the very rapid convergence of the Wigner-Kirkwood expansion for average (nuclear) binding energies.10 p.application/pdfeng(c) The American Physical Society, 1987Teoria quànticaAnàlisi numèricaNumerical analysisQuantum theoryWigner-Kirkwood expansion of the phase-space density for semi-infinite nuclear matterinfo:eu-repo/semantics/article35055info:eu-repo/semantics/openAccess