12C(α,γ)16O Thermonuclear Reaction Rate: Present Status And Perspectives

Details 12C(α,γ)16O Thermonuclear Reaction Rate: Present Status And Perspectives 12C(α,γ)16O Thermonuclear Reaction Rate: Present Status And Perspectives

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1012..150l&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP Conference Proceedings, Volume 1012, pp. 150-154 (

Astronomy and Astrophysics

Astrophysics

Fusion Reactors, Big Bang Nucleosynthesis, Bond Strengths, Dissociation Energies, 6<=A<=19

Scientific paper

I review quite briefly for reasons of length, the reaction 12C(α,γ)16O that follows core hydrogen burning and governs, with the triple-α process, most of the universal abundances of 12C and 16O, including new and previously unpublished work. The present status of the 12C(α,γ) 16O cross section knowledge and its consequences on the reaction rate uncertainties are presented with some perspective to reach the desired precision at stellar temperatures.

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