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208                                              G. P. ARRIGHINI AND C. GUIDOTTI

                              and successively












                              After carrying out the integrations involved in eq. (2.15) [34], we finally obtain the result


                              which allows one to calculate the numerical electronic density in terms of both the
                              potential    characterizing the one-electron model assumed and the electric field
                              polarizing the electron distribution itself. It should be evident from the derivation that the
                              effect of the field  has not been taken into account according to a perturbative
                              treatment; eq. (2.16) is an approximate result for the electron density that includes at
                              infinite order the polarization distortion caused by the external field.
                              Eq. (2.16) is not an entirely new result. After this work had been concluded and we were
                              looking around in search of bibliographical material, we came upon a paper by Englert
                              and Schwinger [24] dealing with the introduction of quantum corrections to the Thomas-
                              Fermi statistical atom. These authors attain the same result expressed by eq. (2.16) (for
                              the case     by resorting to a somewhat more general assumption about the adopted
                              QMP          as compared to our choice.
                              For a quantum system with a single degree of freedom (dimensionality  a procedure
                              parallel to that sketched above leads to the following result


                              where







                              The Fermi level energy  appearing in eq. (2.16) [or eq. (2.17)] through the argument b
                              of the Airy function and its derivative is fixed by the normalization requirement

                              [or the analogous one-dimensional stemming from eq. (2.17)]. Obviously  depends on
                              the external field  amplitude.
                              Unperturbed electron densities descend naturally from the above formalism by letting
                              vanish.
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