Revised V45(p,γ)Cr46 astrophysical reaction rate

Details Revised V45(p,γ)Cr46 astrophysical reaction rate Revised V45(p,γ)Cr46 astrophysical reaction rate

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phrvc..75f8801h&link_type=abstract

Physical Review C, vol. 75, Issue 6, id. 068801

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Nuclear Reaction Models And Methods, Single-Particle Levels And Strength Functions, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 39<=A<=58

Scientific paper

The astrophysical reaction rate of the V45(p,γ)Cr46 reaction,
which is relevant to Ti44 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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