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    Band Structure of Nuclear Levels and Pairing Correlation Interactions

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    The modern theory of superconductivity applied to a statistical model of nuclei predicts the phase transition energy all at 2.73 Mev or so for a wide range of mass number. This transition energy curve is identified with cne of the curves which were found by Sakai from a plot of the number of levels against the excitation energy

    Angular Momentum Distributions in the Thomas-Fermi and Thomas-Fermi-Dirac Models of the Atom

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    The angular momentum distributions in the Thomas-Fermi and Thomas-Fermi-Dirac models of the atom are calculated by an ™i mproved method proposed previously. The maximum energy (El),== for a given orbital angular momentum state is not neglected and is treated as an eigenvalue by the WKB method. The effective central field potentials in terms of the universal approximate Thomas-Fermi function proposed by Latter are utilized. The determination of the maximum energy (El),n,, and, therefore, the number of electrons rzl for a given angular momentum state 2 is greatly facilitated by the term values computed by Latter; The calculated angular momentum distributions are checked with the dia-grams of term values against Z given in the Latter ™s paper to assure that our.pro-posed method prouduces no appreciable error. . Comparing with the empirical data, we then tind that the accuracy of the Thomas-Fermi-Dirac model is far better than that of the Thomas-Fermi model. The prediction of the first appearance of the s, p, d and f electrons by the Thomas-Fermi- Dirac model is almost perfectly exact

    Angular Momentum Distributions in the Atomic Nuclei

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    The problem of how many protons (neutrons) of a given orbital angular mo-mentum Itr are to be found in a nucleus of a given proton number Z (neutron number N) is reinvestigated by means of the improved Thomas-Fermi method. Three kinds of nuclear models are calculated: The types of potentials chosen arc (i) square well potential, (ii)-the Green™s potential, and (iii) the Green™s potential plus 45 times the Thomas-Frenkel spin orbit term. The parameters involved in the potentials are adopted from the paper of Hwang and Yang, which may exactly re-produce the nuclear radii, trends of binding energies, and location of 3s and 4s maxima in the neutron scattering cross section. The eigenvalues calculated by Green are used to simplify the procedure of calculation. The results are then compared with the empirical data compiled by Klinkenbeig. For the last type of potential, the calculation is almost perfectly exact. The first appearance of particles of the next higher angular momentum is almost exact for each model. The puzzle in the Yang™s treatment of the first appearance problem is then solved. The crigin of the appearance of magic numbers in the Yang s calculation is explained in the light of the present theory

    Going Beyond Counting First Authors in Author Co-citation Analysis

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    The present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
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