Abstract
Emission probability of 17−23O and 19−25F isotopes from 290−320122, 292−332124 and 298−326126 eve-even parents were studied by calculating the barrier penetrability, decay constant and decay half-lives using the Coulomb and Proximity potential Model (CPPM). The Q-values are estimated using the WS4 mass model. Clusters like 18,20O, 23,25F show the emission probability from the selected parents with a decay half-life less than the experimental upper limit of 1030 seconds. Neutron shell closure at N = 176 and 184 is identified from the plot of log10T1/2 versus the neutron number of parent nuclei.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
