By V. G. Soloviev (auth.), H. Schopper (eds.)
The homes of nuclear degrees and transitions among them are usually not purely vital for nuclear physicists. The collective phenomena in nuclei are of basic curiosity for the reason that they symbolize a many-body process with extra then debris, yet a lot fewer then in condensed topic difficulties. even though, the information of homes of nuclei are both correct to functions in know-how (e.g. transmutation of parts) or medication and likewise to astrophysics.The current quantity I / 18 A is the 1st of 3 volumes devoted to the power degrees and constitution of nuclei, protecting the sunshine nuclei with Z
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The function f , depending on the nuclear charge and E0 , has been tabulated in [69B3, 69Z, 71G]. There is a great number of allowed β-transitions between proton and neutron in the same subshell which are called superallowed with log f t = 3 ÷ 4. The log f t = 4 ÷ 6 holds for βtransitions between different subshells with the same l value. There are allowed l forbidden βtransitions between the subshells with ∆l = 2 and log f t = 6 ÷ 7. This is, for example, the transitions d3/2 → s1/2 , f5/2 → p3/2 etc.
The one-nucleon transfer reactions belong to the reactions (d,p), (d,t), (α,t), (t,α), (α,3 He), 3 ( He, α) and others. Such reactions can excite only states which have one quasiparticle more (or less) than the initial state; the positions of the remaining quasiparticles must be unchanged. The spectroscopic factors in the independent quasiparticle model in spherical nuclei are the following. 133) for example, for the (d,p) reaction on doubly even target nuclei. 134) for example, for the (d,t) reaction on doubly even target nuclei.
In the first one, the explicit form of the residual interaction is used [68Ku, 95Zh]. In the second one, the residual interaction is phenomenological. At first a set of independent matrix elements of the two-nucleon interaction is extracted from the known spectra of the levels, then these elements can be used for calculation of spectra of other nuclei [65Co, 84Wi, 91Ri]. Recently, there appeared papers that relate these two approaches [94Ca]. In principle, the shell model can give almost the complete solution of the many-nucleon problem, and there is a strong tendency to obtain it with modern computers.