Please use this identifier to cite or link to this item: http://dspace.iitrpr.ac.in:8080/xmlui/handle/123456789/502
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSingh, P.P.-
dc.contributor.authorYadav, A.-
dc.contributor.authorSharma, V.R.-
dc.contributor.authorKumar, R.-
dc.contributor.authorSharma, M.K.-
dc.contributor.authorSingh, B.P.-
dc.contributor.authorSingh, R.P.-
dc.contributor.authorMuralithar, S.-
dc.contributor.authorBhowmik, R.K.-
dc.contributor.authorPrasad, R.-
dc.date.accessioned2016-11-19T10:41:32Z-
dc.date.available2016-11-19T10:41:32Z-
dc.date.issued2016-11-19-
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/502-
dc.description.abstractThe onset and strength of incomplete fusion (ICF) has been studied in the framework of Morgenstern's mass-asymmetry systematics. The fraction of ICF has been deduced in 12C+169Tm system at energies ranging from 1.02V b to 1.64Vb (Vb = 54.94 MeV from the analysis of excitation functions (EFs). It has been found that the ICF starts influencing complete fusion at noticeably lower, β-values (i.e., 0.025 or 2. 5% of c) than that proposed by Morgenstern (i.e., ≈ 6% of c). The fraction of ICF increases with entrance channel mass-asymmetry for individual projectiles, termed as projectile dependent mass-asymmetry (ProMass-) systematics. The proposed ProMass- systematics has withstood all tests that have been done for fairly large number of systems to verify its validness.en_US
dc.language.isoen_USen_US
dc.subjectProjectilesen_US
dc.subjectExcitation functionen_US
dc.subjectIncomplete fusionen_US
dc.subjectMass asymmetriesen_US
dc.subjectAstrophysicsen_US
dc.titleReconciliation of mass-asymmetry systematics for incomplete fusionen_US
dc.typeArticleen_US
Appears in Collections:Year-2015

Files in This Item:
File Description SizeFormat 
Full Text.pdf712.15 kBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.