Proton Distribution Radii of O1624: Signatures of New Shell Closures and Neutron Skin

S. Kaur et al.
Phys. Rev. Lett. 129, 142502 – Published 28 September 2022

Abstract

The root mean square radii of the proton density distribution in O1624 derived from measurements of charge changing cross sections with a carbon target at 900AMeV together with the matter radii portray thick neutron skin for O2224 despite O22,24 being doubly magic. Imprints of the shell closures at N=14 and 16 are reflected in local minima of their proton radii that provide evidence for the tensor interaction causing them. The radii agree with ab initio calculations employing the chiral NNLOsat interaction, though skin thickness predictions are challenged. Shell model predictions agree well with the data.

  • Figure
  • Figure
  • Figure
  • Received 11 May 2022
  • Revised 31 July 2022
  • Accepted 30 August 2022

DOI:https://doi.org/10.1103/PhysRevLett.129.142502

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Click to Expand

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 129, Iss. 14 — 30 September 2022

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
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
×