Published August 14, 2024 | Version v1
Journal article

Extraction of Gamow-Teller strengths in the β+ direction with the (d,He2) reaction in inverse kinematics

  • 1. Facility for Rare Isotope Beams, Michigan State University, East Lansing, Michigan 48824, USA
  • 2. Joint Institute for Nuclear Astrophysics: Center for the Evolution of the Elements, Michigan State University, East Lansing, Michigan 48824, USA
  • 3. Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 4. Universidade da Coruña, Campus Industrial de Ferrol, CITENI, Departamento de Física, Ferrol 15403, Spain
  • 5. Physics Division, Argonne National Laboratory, Lemont, Illinois 60439, USA

Description

The (d,He2) reaction in inverse kinematics has been developed for experiments with rare-isotope beams to constrain electron-capture rates needed for astrophysical simulations of processes in dense nuclear environments such as supernovae and neutron star crusts. The first experiment focused on the measurement of the O14(d,He2) and N13(d,He2) reactions in inverse kinematics, utilizing the active-target time-projection chamber placed in front of the S800 magnetic spectrograph. This work focuses on the experimental and analysis details, and presents the results for the N13(d,He2) reaction, which is important for constraining electron captures rates on N13 in the preexplosion convective phase of Type Ia supernova. The extracted Gamow-Teller transition strengths associated with electron capture on N13 are consistent with those previously obtained from the analog transitions from C13. The successful development of the (d,He2) reaction in inverse kinematics presents a novel opportunity for performing experiments aimed at constraining electron-capture rates in nuclei far from stability.

Additional details

Identifiers

DOI
10.1103/PhysRevC.110.024313;
Crossref Funder ID
10.13039/100000001; 10.13039/100006209; 10.13039/100006132; 10.13039/100007709;

Publishing Information

Journal Title
Physical Review C
Journal Volume
110
Journal Issue
2
Journal Page Range
13 pgs.
ISSN
1089-490X

Optional Information

Copyright
©2024 American Physical Society
Contract/Grant/Project number
PHY-1913554; PHY-2209429; PHY-1430152; PHY-1927130; MRI-0923087; DE-SC0000661; RYC2020-030669; PID2022-142557NA-I00
Notes
Contact Email: Contact author: rahman@frib.msu.edu; Contact Email: Contact author: giraud@frib.msu.edu; Contact Email: Contact author: zegers@frib.msu.edu; Record automatically processed
Funding organization
National Science Foundation; Nuclear Physics; Office of Science; Michigan State University; MCIN/AEI/10.13039/501100011033