K 38 isomer production via fast fragmentation

K. A. Chipps, R. L. Kozub, C. Sumithrarachchi, T. Ginter, T. Baumann, K. Lund, A. Lapierre, A. Villari, F. Montes, S. Jin, K. Schmidt, S. Ayoub, S. D. Pain, D. Blankstein

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

In radioactive ion beam experiments, beams containing isomers can be of interest in probing nuclear structure and informing astrophysical reaction rates. While the production of mixed in-flight ground state and isomer beams using nucleon transfer can be generally understood through distorted wave Born approximation methodology, low-spin isomer production via fast fragmentation is relatively unstudied. To attain a practical understanding of low-spin isomer production using fast fragmentation beams, a test case of K38/K38m was studied at the National Superconducting Cyclotron Laboratory's ReAccelerated Beam facility. Starting from lise++ predictions, the fragmentation momentum distribution was sampled to determine isomer production. In addition, the effects of the gas stopper gradient and charge breeding times were examined. In the case of K38, isomer production peaks at ∼57%. This maximum is observed just off the lise++ predicted optimum magnetic rigidity, with only small losses in beam intensity within a few percent of this optimum rigidity setting. Control of the isomer fraction was also achieved through the modification of charge breeding times. Fast fragmentation appears to be a feasible method for production of low-spin isomeric beams, but additional study is necessary to better describe the mechanism involved.

Original languageEnglish
Article number121301
JournalPhysical Review Accelerators and Beams
Volume21
Issue number12
DOIs
StatePublished - Dec 6 2018

Funding

K. A. C. thanks D. Stracener for helpful discussions in preparing the manuscript. Research was sponsored by the Laboratory Directed Research and Development Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the U.S. Department of Energy. This work was supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Contract No. DE-AC05-00OR22725, and the National Science Foundation under Grant No. PHY-1430152 (JINA Center for the Evolution of the Elements) and Grant No. PHY-1565546 (National Superconducting Cyclotron Laboratory).

FundersFunder number
U.S. Department of Energy
National Science FoundationPHY-1430152, PHY-1565546
Nuclear PhysicsDE-AC05-00OR22725
Oak Ridge National Laboratory
Office of Science

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