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Testing and improvements of gamma-ray strength functions for nuclear model calculations of nuclear data

1999/07/29 by V.A. Plujko, V. A. Plujko, Plujko, V. A.
Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Nuclear Experiment (nucl-ex) #Nuclear Physics and Applications #Nuclear Theory (nucl-th) #Nuclear physics research studies #Nuclear reactor physics and engineering #astro-ph #nucl-ex #nucl-th

paper · pdf · doi:10.48550/arxiv.nucl-th/9907111

LaTeX, 35 pages including 5 PostScipt figures. A Progress Report on the IAEA Contract No. 10308/RO. The misprints in Table 2 of previous version are corrected. The column 3 with values of F is omitted, because these values correspond to nucleus Nd-144 only

openalex publication_date 1999/07/29 · arxiv created 1999/07/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

A closed-form thermodynamic pole approach,TPA, is developed for average description of the E1 radiative strength functions using the microcanonical ensemble for initial states. A semiclassical description of the collective excitation damping in this method is based on modern physical notion on the relaxation processes in Fermi systems.The TPA model gives rather accurate means of simultaneous description of the gamma- decay and photoabsorption strength functions in the medium and heavy nuclei. It is able to cover a relatively wide energy interval, ranging from zeroth gamma-ray energy to values above GDR peak energy, as compared with the others closed-form models for calculation of the E1 strength.

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