Alpha Decay in the Complex-Energy Shell Model

Journal Article · Sun Jan 01 00:00:00 EST 2012 · Physical Review C

DOI:https://doi.org/10.1103/PhysRevC.86.034338· OSTI ID:1091692

Betan, R. Id ^[1]; Nazarewicz, Witold ^[2]

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1. UTK/ORNL/Instituto de Fisica Rosario (CONICET), Argentina
2. UTK/ORNL/University of Warsaw

Background: Alpha emission from a nucleus is a fundamental decay process in which the alpha particle formed inside the nucleus tunnels out through the potential barrier. Purpose: We describe alpha decay of 212Po and 104Te by means of the configuration interaction approach. Method: To compute the preformation factor and penetrability, we use the complex-energy shell model with a separable T = 1 interaction. The single-particle space is expanded in a Woods-Saxon basis that consists of bound and unbound resonant states. Special attention is paid to the treatment of the norm kernel appearing in the definition of the formation amplitude that guarantees the normalization of the channel function. Results: Without explicitly considering the alpha-cluster component in the wave function of the parent nucleus, we reproduce the experimental alpha-decay width of 212Po and predict an upper limit of T1/2 = 5.5 10 7 sec for the half-life of 104Te. Conclusions: The complex-energy shell model in a large valence configuration space is capable of providing a microscopic description of the alpha decay of heavy nuclei having two valence protons and two valence neutrons outside the doubly magic core. The inclusion of proton-neutron interaction between the valence nucleons is likely to shorten the predicted half-live of 104Te.

• Research Organization: Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
• Sponsoring Organization: USDOE Office of Science (SC)
• DOE Contract Number: DE-AC05-00OR22725
• OSTI ID: 1091692
• Journal Information: Physical Review C, Vol. 86, Issue 3; ISSN 0556--2813
• Country of Publication: United States
• Language: English