Structure of 8B from elastic and inelastic 7Be+p scattering

J. P. Mitchell, G. V. Rogachev, E. D. Johnson, L. T. Baby, K. W. Kemper, A. M. Moro, P. Peplowski, A. S. Volya, and I. Wiedenhöver
Phys. Rev. C 87, 054617 – Published 23 May 2013

Abstract

Background: Detailed experimental knowledge of the level structure of light weakly bound nuclei is necessary to guide the development of new theoretical approaches that combine nuclear structure with reaction dynamics.

Purpose: The resonant structure of 8B is studied in this work.

Method: Excitation functions for elastic and inelastic 7Be+p scattering were measured using a 7Be rare isotope beam. Excitation energies ranging between 1.6 and 3.4 MeV were investigated. An R-matrix analysis of the excitation functions was performed.

Results: New low-lying resonances at 1.9, 2.54, and 3.3 MeV in 8B are reported with spin-parity assignment 0+, 2+, and 1+, respectively. Comparison to the time-dependent continuum shell (TDCSM) model and ab initio no-core shell model/resonating-group method (NCSM/RGM) calculations is performed. This work is a more detailed analysis of the data first published as a Rapid Communication. J. P. Mitchell, G. V. Rogachev, E. D. Johnson, L. T. Baby, K. W. Kemper et al., [Phys. Rev. C 82, 011601(R) (2010)].

Conclusions: Identification of the 0+, 2+, 1+ states that were predicted by some models at relatively low energy but never observed experimentally is an important step toward understanding the structure of 8B. Their identification was aided by having both elastic and inelastic scattering data. Direct comparison of the cross sections and phase shifts predicted by the TDCSM and ab initio no-core shell model coupled with the resonating group method is of particular interest and provides a good test for these theoretical approaches.

  • Received 1 March 2013

DOI:https://doi.org/10.1103/PhysRevC.87.054617

©2013 American Physical Society

Authors & Affiliations

J. P. Mitchell1,2,3,*, G. V. Rogachev1,4,†, E. D. Johnson1, L. T. Baby1, K. W. Kemper1, A. M. Moro5, P. Peplowski1,6, A. S. Volya1, and I. Wiedenhöver1

  • 1Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
  • 2Departmento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Vicuña Mackenna 4860, Macul, Santiago, Chile
  • 3Argelander Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
  • 4National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
  • 5Department of Physics, University of Seville, Spain
  • 6Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland 20723, USA

  • *jmitchel@astro.puc.cl
  • grogache@fsu.edu

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Issue

Vol. 87, Iss. 5 — May 2013

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