Cluster structure of O17

S. Yu. Mezhevych, A. T. Rudchik, A. A. Rudchik, O. A. Ponkratenko, N. Keeley, K. W. Kemper, M. Mazzocco, K. Rusek, and S. B. Sakuta
Phys. Rev. C 95, 034607 – Published 16 March 2017

Abstract

The transfer reaction C13(B11,Li7)O17 leading to the ground and several excited states of O17 was investigated at an incident boron beam energy of 45 MeV. The experimental data were analyzed by means of coupled-channel Born approximation calculations and O17=α+C13 spectroscopic factors were extracted from a comparison of the data and the calculations at forward angles. The largest spectroscopic factor obtained was that for the subthreshold 6.356 MeV 1/2+ state, important for the production of neutrons in the stellar environment, and the squared Coulomb modified asymptotic normalization coefficient, C̃2, is consistent with previous determinations. A significant rise in the experimental data at backward scattering angles suggested the possibility of O17=Li6+B11 clustering in some O17 states, including the ground state. However, explicit inclusion of Li6 transfer in the calculations could not explain the observed effect. Compound nucleus calculations suggested that while the backward angle rise could be explained by such processes for two of the populated O17 states other multistep direct processes must contribute significantly to the other two.

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  • Received 19 July 2016
  • Revised 14 February 2017

DOI:https://doi.org/10.1103/PhysRevC.95.034607

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

S. Yu. Mezhevych, A. T. Rudchik, A. A. Rudchik, and O. A. Ponkratenko

  • Institute for Nuclear Research, Ukrainian Academy of Sciences, Prospect Nauki 47, 03680 Kyiv, Ukraine

N. Keeley*

  • National Centre for Nuclear Research, ul. Andrzeja Sołtana 7, PL-05-400 Otwock, Poland

K. W. Kemper

  • Department of Physics, The Florida State University, Tallahassee, Florida 32306, USA

M. Mazzocco

  • Dipartimento di Fisica e Astronomia, Università di Padova, via F. Marzolo 8, I-35131 Padova, Italy and INFN-Sezione di Padova, via F. Marzolo 8, I-35131 Padova, Italy

K. Rusek

  • Heavy Ion Laboratory, University of Warsaw, Pasteura 5A, PL-02-093 Warsaw, Poland

S. B. Sakuta

  • Russian Research Center “Kurchatov Institute”, 123182 Moscow, Russia

  • *Corresponding author: nicholas.keeley@ncbj.gov.pl

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Issue

Vol. 95, Iss. 3 — March 2017

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