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DC Field | Value | Language |
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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 |
Appears in Collections: | Year-2015 |
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