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Title:
Neutron capture rates in the r-process - The role of direct radiative capture
Authors:
Mathews, G. J.; Mengoni, A.; Thielemann, F.-K.; Fowler, W. A.
Affiliation:
AA(California, University, Livermore, CA), AB(Kernforschungszentrum Karlsruhe GmbH, Karlsruhe, Germany), AC(Max-Planck-Institut für Physik und Astrophysik, Munich, Germany), AD(California Institute of Technology, Pasadena, CA)
Publication:
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 270, July 15, 1983, p. 740-745. (ApJ Homepage)
Publication Date:
07/1983
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Absorption Cross Sections, Neutron Cross Sections, Nuclear Fusion, Supernovae, Nuclear Physics, Nuclear Spin, Statistical Analysis, Stellar Models
DOI:
10.1086/161164
Bibliographic Code:
1983ApJ...270..740M

Abstract

The nuclear physics associated with neutron capture along the r-process path is reviewed, and it is noted that the usual statistical assumptions for the capture rates may not be valid. A comparison with statistical model calculations reveals that direct radiative capture may be the dominant reaction mechanism in the vicinity of and beyond the r-process path. The fact that the direct radiative capture mechanism represents a firm lower limit to the nuclear cross section is used to infer an upper limit of 1.5×1020 cm-3 for the critical neutron density necessary to guarantee (n, γ) equilibrium in the r-process.

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