Elastic Coulomb breakup of Na34

G. Singh, Shubhchintak, and R. Chatterjee
Phys. Rev. C 94, 024606 – Published 9 August 2016

Abstract

Background: Na34 is conjectured to play an important role in the production of seed nuclei in the alternate r-process paths involving light neutron rich nuclei very near the β-stability line, and as such, it is important to know its ground state properties and structure to calculate rates of the reactions it might be involved in, in the stellar plasma. Found in the region of ‘island of inversion’, its ground state might not be in agreement with normal shell model predictions.

Purpose: The aim of this paper is to study the elastic Coulomb breakup of Na34 on Pb208 to give us a core of Na33 with a neutron and in the process we try and investigate the one neutron separation energy and the ground state configuration of Na34.

Method: A fully quantum mechanical Coulomb breakup theory within the architecture of post-form finite range distorted wave Born approximation extended to include the effects of deformation is used to research the elastic Coulomb breakup of Na34 on Pb208 at 100 MeV/u. The triple differential cross section calculated for the breakup is integrated over the desired components to find the total cross-section, momentum, and angular distributions as well as the average momenta, along with the energy-angular distributions.

Results: The total one neutron removal cross section is calculated to test the possible ground state configurations of Na34. The average momentum results along with energy-angular calculations indicate Na34 to have a halo structure. The parallel momentum distributions with narrow full widths at half-maxima signify the same.

Conclusion: We have attempted to analyze the possible ground state configurations of Na34 and in congruity with the patterns in the ‘island of inversion’ conclude that even without deformation, Na34 should be a neutron halo with a predominant contribution to its ground state most probably coming from Na33(3/2+) 2p3/2ν configuration. We also surmise that it would certainly be useful and rewarding to test our predictions with an experiment to put stricter limits on its ground state configuration and binding energy.

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  • Received 23 March 2016
  • Revised 3 June 2016

DOI:https://doi.org/10.1103/PhysRevC.94.024606

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

G. Singh1,*, Shubhchintak2,†, and R. Chatterjee1,‡

  • 1Department of Physics, Indian Institute of Technology, Roorkee, 247667, India
  • 2Department of Physics and Astronomy, Texas A&M University, Commerce, TX-75429, USA

  • *gagandph@iitr.ac.in
  • shub.shubhchintak@tamuc.edu
  • rcfphfph@iitr.ac.in

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Issue

Vol. 94, Iss. 2 — August 2016

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