The cross section of14N(n, p)14C at stellar energies and its role as a neutron poison forS-process nucleosynthesis

[1]  W. Fowler,et al.  Thermonuclear reaction rates V , 1988 .

[2]  F. Waanders,et al.  Production and properties of implanted targets , 1987 .

[3]  G. Bogaert,et al.  Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars☆ , 1987 .

[4]  U. Heinemann,et al.  Destruction of26Al in explosive nucleosynthesis , 1986 .

[5]  D. Raine Essays in Nuclear Astrophysics , 1983 .

[6]  M. Niecke,et al.  Angular distributions of neutron polarization from the 14C(p, n)14N and 11B(α, n)14N reactions and R-matrix analysis oF 15N in the excitation-energy range between 11.5 and 12.5 MeV , 1977 .

[7]  J. Ziegler,et al.  Hydrogen Stopping Powers and Ranges in All Elements , 1977 .

[8]  I. Iben Thermal pulses: p-capture, alpha -capture, s-process nucleosynthesis; and convective mixing in a star of intermediate mass. , 1975 .

[9]  M. Arnould,et al.  More about the nucleosynthesis of the nuclei between carbon and neon , 1974 .

[10]  C. H. Johnson,et al.  Interaction of Fast Neutrons with Nitrogen , 1950 .

[11]  F. Thielemann,et al.  Explosive hydrogen burning in novae , 1986 .

[12]  A. Jorissen,et al.  A Parametrized Study of the 13C(α,n)16O Neutron Source , 1986 .

[13]  C. Barnes NUCLEOSYNTHESIS BY CHARGED-PARTICLE REACTIONS. , 1971 .

[14]  L. Ruby,et al.  A SIMPLER APPROACH TO THE GEOMETRICAL EFFICIENCY OF A PARALLEL-DISK SOURCE AND DETECTOR SYSTEM , 1968 .

[15]  A. Cameron New Neutron Sources of Possible Astrophysical Importance. , 1960 .