Year: 2021
Type: article
Abstract: Nuclear state densities are important inputs to statistical models of compound-nucleus reactions. State densities are often calculated with self-consistent mean-field approximations that do not include important correlations and must be augmented with empirical collective enhancement factors. Here, we benchmark the static-path plus random-phase approximation (SPA + RPA) to the state density in a chain of samarium isotopes $^{148\text{--}155}\mathrm{Sm}$ against exact results (up to statistical errors) obtained with the shell-model Monte Carlo (SMMC) method. The SPA + RPA method incorporates all static fluctuations beyond the mean field together with small-amplitude quantal fluctuations around each static fluctuation. Using a pairing plus quadrupole interaction, we show that the SPA + RPA state densities agree well with the exact SMMC densities for both the even- and odd-mass isotopes. For the even-mass isotopes, we also compare our results with mean-field state densities calculated with the finite-temperature Hartree-Fock-Bogoliubov (HFB) approximation. We find that the SPA + RPA repairs the deficiencies of the mean-field approximation associated with broken rotational symmetry in deformed nuclei and with the violation of particle-number conservation in the pairing condensate. In particular, in deformed nuclei the SPA + RPA reproduces the rotational enhancement of the state density relative to the mean-field state density.
Source: Physical Review C
Authors: P. Fanto, Y. Alhassid
Institution: Yale University
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Awards: G1071216263, NUCLEAR THEORY, G122673668, G1286236842, G1677143136, G2900453181, G3083819904, G3876214271, G419881185, G42916606, G4501827968, G498139845, G5076365615, SSAA MANAGEMENT OF STEWARDSHIP SCIENCE GRADUATE FELLOWSHIP AND LABORATORY RESIDENCY GRADUATE FELLOWSHIP PROGRAMS, G7146827954, NUCLEAR THEORY, G969889393
OpenAlex ID: W3081895327
