JINA - Virtual Journal of Nuclear Astrophysics, 10 October 2025
Volume 23, Issue 33 (27 Articles)
- # 4 - Constraining the $^{30}$P($p,gamma)^{31}$S reaction rate in ONe novae via the weak, low-energy, $beta$-delayed proton decay of $^{31}$Cl
- T. Budner (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), M. Friedman (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Racah Institute of Physics, Hebrew University, Jerusalem, Israel), C. Wrede (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), B. A. Brown (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), J. Jos'e (Departament de F'isica, Universitat Polit`ecnica de Catalunya, Barcelona, Spain, Institut d'Estudis Espacials de Catalunya, Universitat Polit`ecnica de Catalunya, Barcelona, Spain), D. P'erez-Loureiro (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA), L. J. Sun (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, School of Physics, Astronomy, Shanghai Jiao Tong University, Shanghai, China), J. Surbrook (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), Y. Ayyad (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Instituto Galego de F'isica de Atlas Enerx'ias, Universidade de Santiago de Compostela, Santiago de Compostela, Spain), D. W. Bardayan (Department of Physics, University of Notre Dame, Notre Dame, USA), K. Chae (Department of Physics, Sungkyunkwan University, Seoul, South Korea), A. A. Chen (Department of Physics, Astronomy, McMaster University, Hamilton, Canada), K. A. Chipps (Physics Division, Oak Ridge National Laboratory, Oak Ridge, USA, Department of Physics, Astronomy, University of Tennessee, Knoxville, USA), M. Cortesi (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA), B. Glassman (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), M. R. Hall (Department of Physics, University of Notre Dame, Notre Dame, USA), M. Janasik (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), J. Liang (Department of Physics, Astronomy, McMaster University, Hamilton, Canada), P. O'Malley (Department of Physics, University of Notre Dame, Notre Dame, USA), E. Pollacco (D'epartement de Physique Nucl'eaire, Institut de Recherche sur les lois Fondamentales de l'Univers, Commissariat `a l'energie atomique et aux 'energies alternatives, Universit'e Paris-Saclay, Gif-sur-Yvette, France), A. Psaltis (Department of Physics, Astronomy, McMaster University, Hamilton, Canada), J. Stomps (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA), T. Wheeler (National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, USA, Department of Physics, Astronomy, Michigan State University, East Lansing, USA)
- https://arxiv.org/abs/2204.05444