Alpha-decay from 44Ti: Microscopic alpha half-life calculation using normalized spectroscopic factor
Abstract
The microscopic description of alpha decay from the nucleons' degree of freedom involves a two-step process. The first consists of the clusterization of neutron and proton pairs; the second involves the tunneling process. A robust protocol for calculating the normalized spectroscopic factor, as defined by Fliessbach, and its error is established and used for calculating the alpha-width for the 0+ states of the nucleus 44Ti. The Gamow Shell Model is used to calculate the structure part of the alpha-decay, while the Gamow wave function determines the reaction part. The conventional and normalized spectroscopic factors are calculated for the ground and excited 0+ states of 44Ti and the alpha-width and half-life of the excited states. A near alpha-threshold state has an alpha half-life of 5 μsec. The normalization does not appreciably modify the ground-state clusterization, while the excited states do. The non-resonant continuum significantly increases the clustering of some of the excited states, particularly the T=2 state. The normalized formation amplitude looks like a single-particle wave function.
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