2014
DOI: 10.1134/s106377881409004x
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On an optical-model description of the relaxation of deep hole states in medium-heavy-mass spherical nuclei

Abstract: The Green's function method is used to formulate the single-quasiparticle dispersive optical model with the aim of semimicroscopically describing the relaxation of deep hole states in medium-heavymass spherical nuclei. The results of the calculations performed on the basis of this model for the 208 Pb parent nucleus are compared with experimental data.

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Cited by 18 publications
(22 citation statements)
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“…1). The same conclusion follows from calculations exploiting a realistic partially self-consistent phenomenological mean field provided that the parameters of this mean field adjusted to describe the observable single-quasiparticle spectra near the Fermi energy [3].…”
Section: Introductionmentioning
confidence: 58%
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“…1). The same conclusion follows from calculations exploiting a realistic partially self-consistent phenomenological mean field provided that the parameters of this mean field adjusted to describe the observable single-quasiparticle spectra near the Fermi energy [3].…”
Section: Introductionmentioning
confidence: 58%
“…W(ε) = W(|E|), where E = ε − μ, and |E| is the single-quasiparticle excitation energy; (ii) the real quantity Δ can be presented as the sum Δ d + Δ p , where the first ("dispersive") term is due to the spreading effect while the second ("potential") term simulates the mean-field energy dependence. Using the above supposition for W(|E|), one gets the dispersive relationship which determines the dispersive part of Δ via W [3,4]:…”
Section: Basic Relationsmentioning
confidence: 99%
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