Reexamining shell-model predictions for the mass of Na17(g.s.)

H. T. Fortune
Phys. Rev. C 90, 067302 – Published 1 December 2014

Abstract

A new shell-model calculation for C17 provides spectroscopic factors for use in a computation of mirror energy differences between C17 and Na17. Results are compared with previous predictions.

  • Received 29 September 2014

DOI:https://doi.org/10.1103/PhysRevC.90.067302

©2014 American Physical Society

Authors & Affiliations

H. T. Fortune

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

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Issue

Vol. 90, Iss. 6 — December 2014

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