Microscopic description of the 13N(p, γ)14O reaction at astrophysical energies
- 1 August 1989
- journal article
- Published by Elsevier in Nuclear Physics A
- Vol. 500 (1) , 155-167
- https://doi.org/10.1016/0375-9474(89)90135-8
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- Study of the 13N(p, γ)14O reaction at stellar energies in a microscopic coupled-channel approachNuclear Physics A, 1987
- Current status of nuclear astrophysicsReports on Progress in Physics, 1987
- Antisymmetrization effects in radiative capture reactionsAnnals of Physics, 1985
- The reaction at stellar energiesNuclear Physics A, 1985
- Calculation of the 13N(p, ?)14O Cross Section at Low EnergiesAustralian Journal of Physics, 1985
- The N-13(p, gamma)O-14 thermonuclear reaction rate and the hot CNO cycleThe Astrophysical Journal, 1984
- Electromagnetic transitions and radiative capture in the generator-coordinate methodNuclear Physics A, 1983
- Microscopic R-matrix theory in a generator coordinate basisNuclear Physics A, 1977
- Chapter II. Theory of Resonating Group Method and Generator Coordinate Method, and Orthogonality Condition ModelProgress of Theoretical Physics Supplement, 1977
- Equilibrium deformation calculations of the ground state energies of 1p shell nucleiNuclear Physics, 1965