JINA - Virtual Journal of Nuclear Astrophysics,
13 March 2026
Volume 24, Issue 11 (16 Articles)
- # 3 - Implications for Type Ia Supernova Nucleosynthesis from an Experimentally Constrained $^{16}$O$(p,alpha)^{13}$N Reaction Rate
- M. Alruwaili (University of York, UK, Northern Border University, Saudi Arabia), C. Fougeres (Argonne National Laboratory, USA), A. M. Laird (University of York, UK), H. Jayatissa (Argonne National Laboratory, USA), M. L. Avila (Argonne National Laboratory, USA), E. Bravo (Universidad de Granada, Spain), C. Angus (University of York, UK, TRIUMF, Canada), C. Badenes (University of Pittsburgh, USA), S. Chakraborty (University of York, UK), C. Diget (University of York, UK), N. de Sereville (Institut de Physique Nucleaire d'Orsay, France), A. Hall-Smith (University of York, UK), R. Longland (North Carolina State University, USA, Triangle Universities Nuclear Laboratory, USA), W. -J. Ong (Lawrence Livermore National Laboratory, USA), K. E. Rehm (Argonne National Laboratory, USA), D. Santiago-Gonzalez (Argonne National Laboratory, USA)
- https://arxiv.org/abs/2603.06307
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.
