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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Main Authors: Norah A.M. Alsaif, Saad M. Saleh Ahmed, H. Al-Ghamdi
Format: Article
Language:English
Published: Elsevier 2020-12-01
Series:Results in Physics
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S2211379720321057
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spelling 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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