Reconciliation of mass-asymmetry systematics for incomplete fusion

Sharma, V.R.; Singh, R.P.; Prasad, R.; Singh, P.P.; Bhowmik, R.K.; Kumar, R.; Muralithar, S.; Singh, B.P.; Sharma, M.K.; Yadav, A.

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dc.contributor.author	Singh, P.P.
dc.contributor.author	Yadav, A.
dc.contributor.author	Sharma, V.R.
dc.contributor.author	Kumar, R.
dc.contributor.author	Sharma, M.K.
dc.contributor.author	Singh, B.P.
dc.contributor.author	Singh, R.P.
dc.contributor.author	Muralithar, S.
dc.contributor.author	Bhowmik, R.K.
dc.contributor.author	Prasad, R.
dc.date.accessioned	2016-11-19T10:41:32Z
dc.date.available	2016-11-19T10:41:32Z
dc.date.issued	2016-11-19
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/502
dc.description.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.	en_US
dc.language.iso	en_US	en_US
dc.subject	Projectiles	en_US
dc.subject	Excitation function	en_US
dc.subject	Incomplete fusion	en_US
dc.subject	Mass asymmetries	en_US
dc.subject	Astrophysics	en_US
dc.title	Reconciliation of mass-asymmetry systematics for incomplete fusion	en_US
dc.type	Article	en_US