Abstract The20Ne(α,p)23Na reaction rate is important in determining the final abundances of various nuclei produced in type Ia supernovae. Previously, the ground state cross section was calculated from time reversal reaction experiments using detailed balance. The reaction rates extracted from these studies do not consider contributions from the population of excited states, and therefore, are only estimates. A resonance scan, populating both the ground and first excited states, was performed for the20Ne(α,p)23Na reaction, measuring between 2.9 and 5 MeV center of mass energies at the Nuclear Science Lab at the University of Notre Dame. Data analysis is underway and preliminary results show substantial contribution from the excited state reaction.
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Atomic autoionization in the photo-dissociation of super-excited deuterated water molecules fragmenting into D + + O + + D
Creation of a super-excited radical water cation results in a long-lived excited oxygen fragment that can act as a destructive carrier and initiate secondary reactions such as breakup of DNA strands – a key radiation damage mechanism.
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- Award ID(s):
- 2208017
- PAR ID:
- 10527355
- Publisher / Repository:
- The Royal Society of Chemistry
- Date Published:
- Journal Name:
- Physical Chemistry Chemical Physics
- Volume:
- 25
- Issue:
- 32
- ISSN:
- 1463-9076
- Page Range / eLocation ID:
- 21562 to 21572
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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