Evaluation of experimental constraints on the Ti44(α,p)V47 reaction cross section relevant for supernovae
Author:
Funder
U.S. Department of Energy
Office of Science
Oak Ridge National Laboratory
National Science Foundation
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.102.035806/fulltext
Reference39 articles.
1. Emission from 44Ti associated with a previously unknown Galactic supernova
2. Detection of the 67.9 and 78.4 [CLC]ke[/CLC]V Lines Associated with the Radioactive Decay of [TSUP]44[/TSUP]T[CLC]i[/CLC] in Cassiopeia A
3. The Signature of 44 Ti in Cassiopeia A Revealed by IBIS/ISGRI on INTEGRAL
4. Asymmetries in core-collapse supernovae from maps of radioactive 44Ti in Cassiopeia A
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1. Production of 44Ti and Iron-group Nuclei in the Ejecta of 3D Neutrino-driven Supernovae;The Astrophysical Journal Letters;2023-11-01
2. Study of the 44Ti(α, p)47V reaction rate using high-precision 50Cr(p, t)48Cr measurements;Journal of Physics: Conference Series;2023-09-01
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