Incomplete fusion in O16+Y89 reactions at energies of 7 MeV/nucleon

Muntazir Gull, Kamal Kumar, Sabir Ali, Tauseef Ahmad, S. Dutt, I. A. Rizvi, Avinash Agarwal, and R. Kumar
Phys. Rev. C 98, 034603 – Published 5 September 2018

Abstract

Measurement of forward recoil range distribution (FRRD) of evaporation residues (ERs) populated in the O16+Y89 reaction at Elab105 MeV have been carried out by employing the offline characteristic γ-ray detection method. The FRRD pattern of ERs populated through xn/pxn channels comprises a single peak only whereas ERs populated through α emitting channel have multiple peaks in their FRRD. FRRDs of the observed ERs support the presence of the complete fusion (CF) process in the population of xn/pxn channels residues and an admixture of complete and incomplete fusion (ICF) processes in the population of α emitting channel residues. The observed ICF process in the population of α emitting channel residues is explained through the breakup fusion model. The fusion function is derived from the experimental CF cross section data and the extracted fusion function is compared with the universal fusion function to estimate the degree of ICF contribution to the total fusion cross section. An attempt has also been made to explore the dependence of ICF probability on target charge.

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  • Received 15 May 2018

DOI:https://doi.org/10.1103/PhysRevC.98.034603

©2018 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Muntazir Gull1,*, Kamal Kumar1, Sabir Ali2,†, Tauseef Ahmad1, S. Dutt1, I. A. Rizvi1, Avinash Agarwal3, and R. Kumar4

  • 1Department of Physics, Aligarh Muslim University, Aligarh, Uttar Pradesh 202 002, India
  • 2MANUU Polytechnic Darbhanga, Maulana Azad National Urdu University, Hyderabad 500 032, India
  • 3Department of Physics, Bareilly College, Bareilly, Uttar Pradesh 243 005, India
  • 4NP-Group, Inter University Accelerator Centre, New Delhi 110 067, India

  • *muntazirgull1@gmail.com
  • sabir@manuu.ac.in

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Issue

Vol. 98, Iss. 3 — September 2018

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