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The waiting point approximation in R-process calculationsThe steady flow approximation to the r-process has been used to evaluate the validity of the waiting point assumption (that, for a given charge number Z, neutron captures become balanced by neutron photodisintegrations) under a variety of conditions. The criterion for the accuracy of the approximation for any set of nuclei with the same value of Z is that the ratio of the total rate of neutron photodisintegration in those nuclei to the total rate of neutron captures should be close to unity. No set of conditions involving neutron production by helium thermonuclear reactions (at temperatures up to 10 to the 9th K) could be found for which the waiting point approximation is useful for all values of Z, and it is recommended that all such r-process calculations not use this approximation. At higher temperatures, such as those characteristic of explosive carbon burning (2 x 10 to the 9th K), the waiting point approximation is much better.
Document ID
19830053324
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cameron, A. G. W.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Cowan, J. J.
(Oklahoma, University Norman, OK, United States)
Truran, J. W.
(Illinois, University Urbana, IL, United States)
Date Acquired
August 11, 2013
Publication Date
April 1, 1983
Publication Information
Publication: Astrophysics and Space Science
Volume: 91
Issue: 2 Ap
ISSN: 0004-640X
Subject Category
Astrophysics
Accession Number
83A34542
Funding Number(s)
CONTRACT_GRANT: NGR-22-007-272
CONTRACT_GRANT: NSF AST-80-19545
CONTRACT_GRANT: NSF AST-80-18198
Distribution Limits
Public
Copyright
Other

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