| Автор | Satish Kumar |
| Автор | J S Batra |
| Автор | Raj K Gupta |
| Дата выпуска | 1996-02-01 |
| dc.description | Cluster emissions from neutron-rich , and nuclei are studied within the preformed cluster model of Malik and Gupta. Q-value estimates of the decays selected on the basis of shell effects in binding energies and their relative preformation probabilities show that these nuclei are stable (Q<0) against and decays and all the metastable (Q>0) decays are of non-alpha-like heavy clusters. The most probable decays (minimum half-life times) are the ones with a doubly magic nucleus as the daughter nucleus, arising due to the WKB penetrability. Compared to the presently measurable alpha-like cluster decays of the corresponding neutron-deficient parents into a daughter nucleus, these decays are suppressed by many orders of magnitude. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Cluster emissions with daughter from neutron-rich nuclei |
| Тип | paper |
| DOI | 10.1088/0954-3899/22/2/006 |
| Electronic ISSN | 1361-6471 |
| Print ISSN | 0954-3899 |
| Журнал | Journal of Physics G: Nuclear and Particle Physics |
| Том | 22 |
| Первая страница | 215 |
| Последняя страница | 219 |
| Аффилиация | Satish Kumar; Department of Physics, Panjab University, Chandigarh-160 014, India |
| Аффилиация | J S Batra; Department of Physics, Panjab University, Chandigarh-160 014, India |
| Аффилиация | Raj K Gupta; Department of Physics, Panjab University, Chandigarh-160 014, India |
| Выпуск | 2 |
