Octupole strength in the neutron-rich calcium isotopes

L. A. Riley, D. M. McPherson, M. L. Agiorgousis, T. R. Baugher, D. Bazin, M. Bowry, P. D. Cottle, F. G. DeVone, A. Gade, M. T. Glowacki, S. D. Gregory, E. B. Haldeman, K. W. Kemper, E. Lunderberg, S. Noji, F. Recchia, B. V. Sadler, M. Scott, D. Weisshaar, and R. G. T. Zegers
Phys. Rev. C 93, 044327 – Published 22 April 2016; Erratum Phys. Rev. C 93, 069902 (2016)

Abstract

Low-lying excited states of the neutron-rich calcium isotopes Ca4852 have been studied via γ-ray spectroscopy following inverse-kinematics proton scattering on a liquid hydrogen target using the GRETINA γ-ray tracking array. The energies and strengths of the octupole states in these isotopes are remarkably constant, indicating that these states are dominated by proton excitations.

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  • Received 1 March 2016

DOI:https://doi.org/10.1103/PhysRevC.93.044327

©2016 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Erratum

Erratum: Octupole strength in the neutron-rich calcium isotopes [Phys. Rev. C 93, 044327 (2016)]

L. A. Riley, D. M. McPherson, M. L. Agiorgousis, T. R. Baugher, D. Bazin, M. Bowry, P. D. Cottle, F. G. DeVone, A. Gade, M. T. Glowacki, S. D. Gregory, E. B. Haldeman, K. W. Kemper, E. Lunderberg, S. Noji, F. Recchia, B. V. Sadler, M. Scott, D. Weisshaar, and R. G. T. Zegers
Phys. Rev. C 93, 069902 (2016)

Authors & Affiliations

L. A. Riley1, D. M. McPherson2, M. L. Agiorgousis1, T. R. Baugher3,4, D. Bazin3, M. Bowry3,4, P. D. Cottle2, F. G. DeVone1, A. Gade3,4, M. T. Glowacki1, S. D. Gregory1, E. B. Haldeman1, K. W. Kemper2, E. Lunderberg3,4, S. Noji3,5, F. Recchia3,*, B. V. Sadler1, M. Scott3,4, D. Weisshaar3, and R. G. T. Zegers3,4,5

  • 1Department of Physics and Astronomy, Ursinus College, Collegeville, Pennsylvania 19426, USA
  • 2Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
  • 3National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
  • 4Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 5Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements, Michigan State University, East Lansing, Michigan 48824, USA

  • *Dipartimento di Fisica e Astronomia Galileo Galilei, Universita degli Studi di Padova, I-35131 Padova, Italy.

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Issue

Vol. 93, Iss. 4 — April 2016

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