• Featured in Physics
  • Editors' Suggestion

Location of the Neutron Dripline at Fluorine and Neon

D. S. Ahn, N. Fukuda, H. Geissel, N. Inabe, N. Iwasa, T. Kubo, K. Kusaka, D. J. Morrissey, D. Murai, T. Nakamura, M. Ohtake, H. Otsu, H. Sato, B. M. Sherrill, Y. Shimizu, H. Suzuki, H. Takeda, O. B. Tarasov, H. Ueno, Y. Yanagisawa, and K. Yoshida
Phys. Rev. Lett. 123, 212501 – Published 18 November 2019
Physics logo See Viewpoint: Reaching the Limits of Nuclear Existence

Abstract

A search for the heaviest isotopes of fluorine, neon, and sodium was conducted by fragmentation of an intense Ca48 beam at 345MeV/nucleon with a 20-mm-thick beryllium target and identification of isotopes in the large-acceptance separator BigRIPS at the RIKEN Radioactive Isotope Beam Factory. No events were observed for F32,33, Ne35,36, and Na38 and only one event for Na39 after extensive running. Comparison with predicted yields excludes the existence of bound states of these unobserved isotopes with high confidence levels. The present work indicates that F31 and Ne34 are the heaviest bound isotopes of fluorine and neon, respectively. The neutron dripline has thus been experimentally confirmed up to neon for the first time since O24 was confirmed to be the dripline nucleus nearly 20 years ago. These data provide new keys to understanding the nuclear stability at extremely neutron-rich conditions.

  • Figure
  • Figure
  • Figure
  • Received 28 March 2019

DOI:https://doi.org/10.1103/PhysRevLett.123.212501

© 2019 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Viewpoint

Key Image

Reaching the Limits of Nuclear Existence

Published 18 November 2019

Researchers have identified the largest possible isotopes of fluorine and neon, extending the neutron “dripline” for the first time in 20 years.

See more in Physics

Authors & Affiliations

D. S. Ahn1, N. Fukuda1, H. Geissel5, N. Inabe1, N. Iwasa4, T. Kubo1,*,†, K. Kusaka1, D. J. Morrissey6, D. Murai3, T. Nakamura2, M. Ohtake1, H. Otsu1, H. Sato1, B. M. Sherrill6, Y. Shimizu1, H. Suzuki1, H. Takeda1, O. B. Tarasov6, H. Ueno1, Y. Yanagisawa1, and K. Yoshida1

  • 1RIKEN Nishina Center for Accelerator-Based Science, RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
  • 2Department of Physics, Tokyo Institute of Technology, 2-12-1 O-Okayama, Meguro, Tokyo 152-8551, Japan
  • 3Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan
  • 4Department of Physics, Tohoku University, 6-3, Aramaki Aza-Aoba, Aoba-ku, Sendai, Miyagi 980-8578, Japan
  • 5GSI, Helmholtzzentrum für Schwerionenforschung GmbH, Planckstraße 1, 64291 Darmstadt, Germany
  • 6National Superconducting Cyclotron Laboratory, Michigan State University, 640 South Shaw Lane, East Lansing, Michigan 48824, USA

  • *Corresponding author. kubo@ribf.riken.jp
  • Present address: Facility for Rare Isotope Beams, Michigan State University, 640 South Shaw Lane, East Lansing, Michigan 48824, USA.

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 123, Iss. 21 — 22 November 2019

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
×