(α,γOE2 cross section in a microscopic four-alpha model
- 1 January 1993
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review C
- Vol. 47 (1) , 210-215
- https://doi.org/10.1103/physrevc.47.210
Abstract
The (α,γO E2 cross section is calculated in the generator coordinate method where is described by three α particles located on the apexes of an equilateral triangle. Distortion effects in the wave functions are taken into account, and the wave functions are defined by a mixing of αC(,) configurations. The good quantum numbers are restored through angular momentum projection. We compute quadrupole transition probabilities between low-energy states, and the (α,γO E2 cross sections to the ground and states. At 300 keV, we find an S factor equal to 0.09 MeV b.
Keywords
This publication has 17 references indexed in Scilit:
- The 12C(a,g)16O Cross Section at Low EnergiesAustralian Journal of Physics, 1991
- K-matrix analysis of theC12(α,γ) reaction at low energyPhysical Review C, 1989
- Coincidence measurement of theC(α,γO cross section at low energiesPhysical Review Letters, 1988
- The scattering of alpha particles from 12C and the stellar reaction rateNuclear Physics A, 1987
- The 12C(a,?)16O Cross Section at Stellar EnergiesAustralian Journal of Physics, 1987
- The 12C(α, γ)16O cross section at stellar energiesNuclear Physics A, 1987
- 12C(α,γ)16O revisitedNuclear Physics A, 1985
- The E2 contribution to the reaction at stellar energies in a coupled channel approachPhysics Letters B, 1985
- Microscopic analysis of the 12C(α, γ)16O reactionNuclear Physics A, 1984
- The 12C(α, γ)16O reaction and stellar helium burningNuclear Physics A, 1974