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AbstractAbstract
[en] The astrophysical reaction rate of the 45V(p,γ)46Cr reaction, which is relevant to 44Ti production in core-collapse supernovae, has been revised through a consistent application of the Thomas-Ehrman level displacement formalism. The new rate agrees well with that predicted by the NON-SMOKER statistical calculation with an ETFSI mass model
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Source
(c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
Record Type
Journal Article
Journal
Country of publication
BARYON REACTIONS, BETA DECAY RADIOISOTOPES, BETA-PLUS DECAY RADIOISOTOPES, BINARY STARS, CHARGED-PARTICLE REACTIONS, CHROMIUM ISOTOPES, ELECTRON CAPTURE RADIOISOTOPES, ERUPTIVE VARIABLE STARS, EVEN-EVEN NUCLEI, HADRON REACTIONS, INTERMEDIATE MASS NUCLEI, ISOTOPES, KINETICS, MATHEMATICAL MODELS, MILLISECONDS LIVING RADIOISOTOPES, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, ODD-EVEN NUCLEI, RADIOISOTOPES, STARS, TITANIUM ISOTOPES, VANADIUM ISOTOPES, VARIABLE STARS, YEARS LIVING RADIOISOTOPES
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