Journal
PHYSICAL REVIEW C
Volume 89, Issue 3, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.89.035802
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Funding
- National Natural Science Foundation of China [11135005, U1232208]
- Major State Basic Research Development Program of China [2013CB834406, 2013CB834401]
- Spanish MICINN [AYA2010-15685, EUI2009-04167]
- E.U. FEDER funds
- ESF EUROCORES Program EuroGENESIS
- NSF [PHY-1068217]
- Swiss NSF
- EuroGENESIS
- ENSAR/THEXO Collaboration within the 7th Framework Programme of the EU
- Division Of Physics
- Direct For Mathematical & Physical Scien [1068217] Funding Source: National Science Foundation
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The thermonuclear rate of the Ti-42(p, gamma)V-43 reaction has been reevaluated based on a recent precise proton separation energy measurement of S-p(V-43) = 83 +/- 43 keV. The astrophysical impact of our new rates has been investigated through one-zone postprocessing type-I x-ray burst calculations. It shows that the new experimental value of S-p significantly affects the yields of species for A approximate to 40-45. As well, the precision of the recent experimental S-p value constrains these yields to better than a factor of 3.
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