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Steady flow approximations to the helium r-processA steady flow approximation to the r-process is presented and used for numerical experiments with physical quantities to determine the sensitivity of the process to variations in those quantities. The effect of neutron capture cross sections along the capture path and of recently available improved beta decay rates on the r-process are discussed. The peaks in the observed r-process yield curve near mass numbers 80 and 130 are roughly characterized by a neutron number density of 10 to the 20th per cu/cm; the mean beta decay rates are about 10/s, and the freezing time is comparable to or less than 0.1 s. The peak near mass number 195 is roughly characterized by a neutron number density of 10 to the 21st/cm, the mean beta decay rates are about 100/s, and the freezing time is comparable to or less than 0.01 s. The flow path of the steady state r-process is sensitively dependent upon the neutron capture cross sections in the flow network and on the values of the beta decay rates.
Document ID
19830053323
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)
Klapdor, H. V.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Metzinger, J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Oda, T.
(Max-Planck-Institut fuer Kernphysik Heidelberg, Germany)
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
83A34541
Funding Number(s)
CONTRACT_GRANT: NSF AST-81-19545
CONTRACT_GRANT: NGR-22-007-272
CONTRACT_GRANT: NSF AST-80-18198
Distribution Limits
Public
Copyright
Other

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