Abstract
The existence of long lived superheavy nuclei (SHN) is controlled mainly by spontaneous fission and α-decay processes. According to microscopic nuclear theory, spherical shell effects at , 120, 126 and provide the extra stability to such SHN to have long enough lifetime to be observed. To investigate whether the so-called “stability island” could really exist around the above , values, the α-decay half-lives along with the spontaneous fission and β-decay half-lives of such nuclei are studied. The α-decay half-lives of SHN with –120 are calculated in a quantum tunneling model with DDM3Y effective nuclear interaction using values from three different mass formulas prescribed by Koura-Uno-Tachibana-Yamada (KUTY), Myers-Swiatecki (MS), and Muntian-Hofmann-Patyk-Sobiczewski (MMM). Calculation of spontaneous fission (SF) half-lives for the same SHN are carried out using a phenomenological formula and compared with SF half-lives predicted by Smolanczuk et al. A possible source of discrepancy between the calculated α-decay half-lives of some nuclei and the experimental data of GSI, JINR-FLNR, RIKEN, is discussed. In the region of –108 with 160–164, the β-stable SHN is predicted to have highest α-decay half-life ( h) using value from MMM. Interestingly, it is much greater than the recently measured ( s) of deformed doubly magic nucleus. A few fission-survived long-lived SHN which are either β-stable or having large β-decay half-lives are predicted to exist near , , , and . These nuclei might decay predominantly through α-particle emission.
- Received 13 August 2007
DOI:https://doi.org/10.1103/PhysRevC.77.044603
©2008 American Physical Society