Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4
The calculations were carried out using an energy-dependent formula, where the superheavy-nuclei mass defect was evaluated by using both the KTUY05 and WS4 nuclear mass formulae. This formula reproduced successfully the value of 212Pocalculated from a combined microscopic shell and cluster model and...
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doaj-3beec1c7f58249a7bce3024956ace8cb2021-01-05T09:21:41ZengElsevierResults in Physics2211-37972020-12-0119103689Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4Norah A.M. Alsaif0Saad M. Saleh Ahmed1H. Al-Ghamdi2Physics Department, Faculty of Science, Princess Nourah Bint Abdulrahman University, Riyadh, Kingdom Saudi Arabia; Corresponding author.Department of Physics, College of Science, University of Baghdad, IraqPhysics Department, Faculty of Science, Princess Nourah Bint Abdulrahman University, Riyadh, Kingdom Saudi ArabiaThe calculations were carried out using an energy-dependent formula, where the superheavy-nuclei mass defect was evaluated by using both the KTUY05 and WS4 nuclear mass formulae. This formula reproduced successfully the value of 212Pocalculated from a combined microscopic shell and cluster model and described satisfactorily the alpha decay of heavy nuclei. The values of the preformation probability and the cluster formation energy, and their dependence on the neutron number, confirmed the shell and subshell closures and the similarities of alpha clustering between heavy and superheavy nuclei. The calculations carried out with the WS4 mass formula showed larger alpha-clustering effects than the KTUY05.http://www.sciencedirect.com/science/article/pii/S2211379720321057Alpha preformation probabilityCluster modelSuperheavy nucleiAlpha clusterPreformation factorBinding energies |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Norah A.M. Alsaif Saad M. Saleh Ahmed H. Al-Ghamdi |
spellingShingle |
Norah A.M. Alsaif Saad M. Saleh Ahmed H. Al-Ghamdi Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4 Results in Physics Alpha preformation probability Cluster model Superheavy nuclei Alpha cluster Preformation factor Binding energies |
author_facet |
Norah A.M. Alsaif Saad M. Saleh Ahmed H. Al-Ghamdi |
author_sort |
Norah A.M. Alsaif |
title |
Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4 |
title_short |
Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4 |
title_full |
Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4 |
title_fullStr |
Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4 |
title_full_unstemmed |
Alpha clustering preformation probability in even-even and odd-A270−317(116 and 117) using cluster formation model and the mass formulae : KTUY05 and WS4 |
title_sort |
alpha clustering preformation probability in even-even and odd-a270−317(116 and 117) using cluster formation model and the mass formulae : ktuy05 and ws4 |
publisher |
Elsevier |
series |
Results in Physics |
issn |
2211-3797 |
publishDate |
2020-12-01 |
description |
The calculations were carried out using an energy-dependent formula, where the superheavy-nuclei mass defect was evaluated by using both the KTUY05 and WS4 nuclear mass formulae. This formula reproduced successfully the value of 212Pocalculated from a combined microscopic shell and cluster model and described satisfactorily the alpha decay of heavy nuclei. The values of the preformation probability and the cluster formation energy, and their dependence on the neutron number, confirmed the shell and subshell closures and the similarities of alpha clustering between heavy and superheavy nuclei. The calculations carried out with the WS4 mass formula showed larger alpha-clustering effects than the KTUY05. |
topic |
Alpha preformation probability Cluster model Superheavy nuclei Alpha cluster Preformation factor Binding energies |
url |
http://www.sciencedirect.com/science/article/pii/S2211379720321057 |
work_keys_str_mv |
AT norahamalsaif alphaclusteringpreformationprobabilityinevenevenandodda270317116and117usingclusterformationmodelandthemassformulaektuy05andws4 AT saadmsalehahmed alphaclusteringpreformationprobabilityinevenevenandodda270317116and117usingclusterformationmodelandthemassformulaektuy05andws4 AT halghamdi alphaclusteringpreformationprobabilityinevenevenandodda270317116and117usingclusterformationmodelandthemassformulaektuy05andws4 |
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1724348413347102720 |