Alpha-decay from Ti: A study of the microscopic clusterization
arXiv:2310.13428 · doi:10.1103/PhysRevC.108.044314
Abstract
Microscopic determination of alpha-decay half-lives requires structure and reaction calculations. The structure part is given by the microscopic distribution of the constituent nucleons, while the relative motion of the product's decay provides the reaction part. This paper studies the clusterization of the excited states of Ti arising from the nucleonic degrees of freedom. The continuum spectra of proton and neutron are incorporated through the Gamow Shell Model formalism. The alpha-like wave function is calculated in the weak-coupling approximation. Gaussian effective interaction in each pair of nucleons is included. The ground and excited states are compared with experiment and shell model calculations. The wave function amplitudes are obtained and discriminated by their resonant and non-resonant contributions. The influence of a four-body truncated basis is analyzed. Inclusion of the continuum spectra produces a gain in the excited states of a few hundred keV of energy. One candidate for alpha decay was identified near the experimental unresolved state of 6.8 MeV excitation energy, with a lower limit for the half-life of ns.
arXiv comment8 pages, 3 figures, 9 tables, 35 references
References in corpus (9)
- Gamow Shell Model Description of Neutron-Rich Nuclei
- Two-Particle Resonant States in a Many-Body Mean Field
- Nuclear Reactions Rates Governing the Nucleosynthesis of Ti44
- Quantified Gamow Shell Model interaction for -shell nuclei
- Alpha Decay in the Complex Energy Shell Model
- Shell model in the complex energy plane and two-particle resonances
- The 40Ca(alpha,gamma)44Ti reaction in the energy regime of supernova nucleosynthesis
- Primary gamma-ray spectra in 44Ti of astrophysical interest
- Direct determination of the neutron skin thicknesses in Ca from proton elastic scattering at MeV