Clustering effects and decay analysis of the light-mass N=Z and NZ composite systems formed in heavy ion collisions

Manpreet Kaur, BirBikram Singh, S. K. Patra, and Raj K. Gupta
Phys. Rev. C 95, 014611 – Published 26 January 2017

Abstract

We investigate the clustering effects in light mass N=Z and NZ composite systems Ne*20, Si*28, Ca*40 and Ne*21,22, K*39, respectively, formed in low-energy heavy ion reactions at different excitation energies, within the collective clusterization approach of the dynamical cluster-decay model (DCM) of Gupta and collaborators based on quantum-mechanical fragmentation theory (QMFT). Considering quadrupole deformed and compact orientated nuclei, a comparative decay analysis of these systems has been undertaken for the emission of different intermediate mass fragments (IMFs) or clusters, specifically the IMFs having Z=3, 4, and 5 (or Z=7, 6, and 5 complimentary fragments from the Ne*20 and Ne*21,22 composite systems) which are having the experimental data available for their Z distribution. Quite interestingly, the QMFT supports clustering in N=Z (Ne*20 and Si*28) and NZ (Ne*21 and Ne*22) nuclear systems at excitation energies corresponding to their respective decay threshold or resonant-state energies for the 4α, O16 cluster and non-α cluster C14 (more so in Ne*22NZ composite system), supported by the Ikeda diagrams, taking into account the proper pairing strength in the temperature-dependent liquid drop energies. Within the DCM, we notice that at higher excitation energies in addition to xα-type (where x is an integer) clusters from N=Z composite systems and xnxα-type clusters from NZ composite systems, npxα-type clusters are relatively quite dominant, with larger preformation probability due to the decreased pairing strength at higher temperatures in the liquid drop energies. Also, the study reveals the presence of competing reaction mechanisms of compound nucleus (fusion-fission, FF) and of noncompound nucleus origin (deep inelastic orbiting, DIO) in the decay of very-light-mass composite systems Ne*20,21,22 and Si*28 at different excitation energies. The DIO contribution in the IMF cross section σIMF is extracted for these composite systems, σIMF is given as the sum of FF cross section σFF and DIO cross section σDIO. The DCM calculated FF cross sections σFFDCM are in good agreement with the available experimental data.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
2 More
  • Received 20 September 2016
  • Revised 19 November 2016

DOI:https://doi.org/10.1103/PhysRevC.95.014611

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Manpreet Kaur1, BirBikram Singh1,*, S. K. Patra2, and Raj K. Gupta3

  • 1Department of Physics, Sri Guru Granth Sahib World University, Fatehgarh Sahib-140406, India
  • 2Institute of Physics, Sachivalaya Marg, Bhubaneswar-751005, India
  • 3Department of Physics, Panjab University, Chandigarh-160014, India

  • *birbikramsingh@sggswu.edu.in

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 95, Iss. 1 — January 2017

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×