Investigation of Sub-Coulomb barrier fusion reaction of ? + 4 0 Ca in different models

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dc.contributor.authorKoyuncu F.
dc.contributor.authorSoylu A.
dc.date.accessioned2019-08-01T13:38:39Z
dc.date.available2019-08-01T13:38:39Z
dc.date.issued2017
dc.departmentNiğde ÖHÜ
dc.description.abstractIn this study, microscopic nucleon-nucleon Double Folding (DF) and phenomenological potentials have been used to investigate ? +40Ca reaction observables at sub-barrier energies. In the calculations, semi-classical Wentzel-Kramers-Brillouin (WKB) approach has been used in order to obtain the cross-sections and reaction rates of ? +40Ca. Besides WKB approximation, we have also utilized Talys code in order to get the comparative results and find out the method differences. To estimate the reaction rates, energy-dependent cross-sections and astrophysical S-factors of ?+40Ca have been used. Herewith, differences between models and potentials have been demonstrated using the reaction rate estimates. © 2017 World Scientific Publishing Company.
dc.description.sponsorshipThis work was supported by the Turkish Science and Research Council (TÜBİTAK) with Grant Number 117R015.
dc.identifier.doi10.1142/S0218301317500860
dc.identifier.issn0218-3013
dc.identifier.issue12
dc.identifier.scopus2-s2.0-85039167111
dc.identifier.scopusqualityQ3
dc.identifier.urihttps://dx.doi.org/10.1142/S0218301317500860
dc.identifier.urihttps://hdl.handle.net/11480/1765
dc.identifier.volume26
dc.identifier.wosWOS:000419375100007
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.institutionauthor[0-Belirlenecek]
dc.language.isoen
dc.publisherWorld Scientific Publishing Co. Pte Ltd
dc.relation.ispartofInternational Journal of Modern Physics E
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectAstrophysical S-factor
dc.subjectreaction rate
dc.subjectWKB method
dc.titleInvestigation of Sub-Coulomb barrier fusion reaction of ? + 4 0 Ca in different models
dc.typeArticle

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