Published 1989 | Version v1
Book

Fission in the astrophysical r-process

  • 1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  • 2. Univ. of Oklahoma, Norman (United States)

Description

Areas in the nuclear chart where neutron-induced and β--delayed fission are of importance are identified and methods to predict their values are discussed. Presently available theoretical fission barrier heights seem to over-estimate both processes, in comparison to experimental information. Therefore, a judgment of the extent to which they affect r-process calculations can only be preliminary. The authors expect that the influence on the chronometer ratios 232Th/238U and 235U/238U is small. Whether nuclei heavier than Z = 100 can be produced in the r-process can only be decided after calculations with improved mass formulas and fission barrier heights

Additional details

Publishing Information

Publisher
American Nuclear Society, Inc.
Imprint Place
La Grange Park, IL (United States)
Imprint Title
Fifty years with nuclear fission. Volume 2
Imprint Pagination
493 p.
Journal Page Range
p. 592-600.

Conference

Title
Fifty years with nuclear fission.
Dates
25-28 Apr 1989.
Place
Gaithersburg, MD (United States).

Optional Information

Secondary number(s)
CONF-890406--Vol.2.