Update on matter radii of O1724

H. T. Fortune
Phys. Rev. C 97, 054309 – Published 9 May 2018

Abstract

The appearance of new theoretical papers concerning matter radii of neutron-rich oxygen nuclei has prompted a return to this problem. New results provide no better agreement with experimental values than did previous calculations with a simple model. I maintain that there is no reason to adjust the O22 core in the O24 nucleus, and the case of O24 should be reexamined experimentally.

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  • Received 17 February 2018

DOI:https://doi.org/10.1103/PhysRevC.97.054309

©2018 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

H. T. Fortune

  • Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

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Issue

Vol. 97, Iss. 5 — May 2018

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