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Continuum and three-nucleon force effects on Be9 energy levels

Joachim Langhammer, Petr Navrátil, Sofia Quaglioni, Guillaume Hupin, Angelo Calci, and Robert Roth
Phys. Rev. C 91, 021301(R) – Published 5 February 2015
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Abstract

We extend the recently proposed ab initio no-core shell model with continuum to include three-nucleon (3N) interactions beyond the few-body domain. The extended approach allows for the assessment of effects of continuum degrees of freedom as well as of the 3N force in ab initio calculations of structure and reaction observables of p- and lower-sd-shell nuclei. As a first application we concentrate on energy levels of the Be9 system for which all excited states lie above the n-Be8 threshold. For all energy levels, the inclusion of the continuum significantly improves the agreement with experiment, which was an issue in standard no-core shell model calculations. Furthermore, we find the proper treatment of the continuum indispensable for reliable statements about the quality of the adopted 3N interaction from chiral effective field theory. In particular, we find the 12+ resonance energy, which is of astrophysical interest, in good agreement with experiment.

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  • Received 29 October 2014

DOI:https://doi.org/10.1103/PhysRevC.91.021301

©2015 American Physical Society

Authors & Affiliations

Joachim Langhammer1,*, Petr Navrátil2,†, Sofia Quaglioni3, Guillaume Hupin3,‡, Angelo Calci1,2, and Robert Roth1,§

  • 1Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany
  • 2TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, V6T 2A3, Canada
  • 3Lawrence Livermore National Laboratory, P.O. Box 808, L-414, Livermore, California 94551, USA

  • *joachim.langhammer@physik.tu-darmstadt.de
  • navratil@triumf.ca
  • Present address: Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA.
  • §robert.roth@physik.tu-darmstadt.de

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Issue

Vol. 91, Iss. 2 — February 2015

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