Coincidence measurement of theC(α,γO cross section at low energies
- 11 April 1988
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 60 (15) , 1475-1478
- https://doi.org/10.1103/physrevlett.60.1475
Abstract
The E1 capture cross section for the reaction (α,γO to the ground state has been measured for 3.00 MeV. A γ-ray–recoil-particle coincidence technique has been used to obtain essentially background-free reaction yields. A three-level R-matrix analysis of the E1 S factor leads to an allowed range for at 300 keV of 0.00–0.14 MeV b. A model-dependent R-matrix analysis and a hybrid R-matrix analysis result in values of 0.14 and 0.08 MeV b, respectively, for (300).
Keywords
This publication has 19 references indexed in Scilit:
- Nuclear Reactions in StarsAnnual Review of Nuclear and Particle Science, 1986
- Capture Amplitudes in the Reactionat Stellar EnergiesPhysical Review Letters, 1985
- Hydrostatic Nucleosynthesis - Part Two - Core Neon to Silicon Burning and Presupernova Abundance Yields of Massive StarsThe Astrophysical Journal, 1985
- Hydrostatic nucleosynthesis. I - Core helium and carbon burning.The Astrophysical Journal, 1985
- Microscopic analysis of the 12C(α, γ)16O reactionNuclear Physics A, 1984
- Experimental and theoretical nuclear astrophysics: the quest for the origin of the elementsReviews of Modern Physics, 1984
- The 12C(α, γ)16O reaction at stellar energiesNuclear Physics A, 1983
- Microscopic investigation of radiative capture reactionPhysics Letters B, 1983
- The4He(12C, ?)16O reaction at stellar energiesThe European Physical Journal A, 1982
- The 12C(α, γ)16O reaction and stellar helium burningNuclear Physics A, 1974