Charge Radius Isotope Shift Across the N=126 Shell Gap

P. M. Goddard, P. D. Stevenson, and A. Rios
Phys. Rev. Lett. 110, 032503 – Published 15 January 2013

Abstract

We revisit the problem of the kink in the charge radius shift of neutron-rich even isotopes near the N=126 shell closure. We show that the ability of a Skyrme force to reproduce the isotope shift is determined by the occupation of the neutron 1i11/2 orbital beyond N=126 and the corresponding change it causes to deeply-bound protons orbitals with a principal quantum number of 1. Given the observed position of the single-particle energies, one must either ensure occupation is allowed through correlations, or not demand that the single-particle energies agree with experimental values at the mean-field level.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Received 9 October 2012

DOI:https://doi.org/10.1103/PhysRevLett.110.032503

© 2013 American Physical Society

Authors & Affiliations

P. M. Goddard, P. D. Stevenson, and A. Rios

  • Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 110, Iss. 3 — 18 January 2013

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Letters

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×