Please use this identifier to cite or link to this item: http://dspace.iitrpr.ac.in:8080/xmlui/handle/123456789/502
Title: Reconciliation of mass-asymmetry systematics for incomplete fusion
Authors: Singh, P.P.
Yadav, A.
Sharma, V.R.
Kumar, R.
Sharma, M.K.
Singh, B.P.
Singh, R.P.
Muralithar, S.
Bhowmik, R.K.
Prasad, R.
Keywords: Projectiles
Excitation function
Incomplete fusion
Mass asymmetries
Astrophysics
Issue Date: 19-Nov-2016
Abstract: The 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.
URI: http://localhost:8080/xmlui/handle/123456789/502
Appears in Collections:Year-2015

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