Titlebook: Computational Nuclear Physics 1; Nuclear Structure K. Langanke,Joachim A. Maruhn,S. E. Koonin Textbook 1991 Springer-Verlag Berlin Heidelbe

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Electron-Scattering Form Factors and Nuclear Transition Densities,nd comparing them to those extracted from the (e,e’) results, if the latter are available. Otherwise the densities can be used to calculate the (e,e’) cross sections (or form factors) and then these can be compared to the measured data.

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Textbook 1991el or method are discussed together with the numerical methods employed. Instructions for the use of each code, and how to adapt them to local compilers and/or operating systems if necessary, are included.

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The Nuclear Shell Model,s with our best understanding of the sd shell nuclei. To this day, it remains a fundamental approach in nuclear, atomic, and nonrelativistic quark physics, and it is considered a fundamental theoretical starting point in the derivation of most models applying to larger nuclei. As a numerical scheme,

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,The Skyrme—Hartree—Fock Model of the Nuclear Ground State,n applied to a great variety of phenomena, including deformation properties, superheavy nuclei, vibrations, and heavy-ion collisions [2.2]. Nonetheless, their most straightforward application, the description of the ground state of spherical nuclei, remains a useful tool. It serves as the basis for

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The Random-Phase Approximation for Collective Excitations,cation of the method by Bohm and Pines [4.1] to the plasma oscillations of an electron gas. The theory is equivalent to a limit of timedependent Hartree—Fock theory in which the amplitude of the motion is small. Consequently, the applicability of the theory is restricted to systems where a Hartree—F

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Variational Monte Carlo Techniques in Nuclear Physics,ularly within nuclear physics [9.1–4]. The most important applications in nuclear physics are to few-body systems, either at the nucleón or the quark level. A variety of nuclear properties have been calculated with Monte Carlo methods, including the binding energies, electromagnetic form factors, re