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Thermonuclear Reaction Rates

Fowler, William A. and Caughlan, Georgeanne R. and Zimmermann, Barbara A. (1967) Thermonuclear Reaction Rates. Annual Review of Astronomy and Astrophysics, 5 . pp. 525-570. ISSN 0066-4146. http://resolver.caltech.edu/CaltechAUTHORS:20161019-081138741

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Abstract

Modern computer technology has revolutionized theoretical calculations on stellar structure and stellar evolution. Physical information of great complexity, previously ignored or crudely treated, can now be introduced in detail into stellar computations and can be treated with great precision and completeness. In particular it is no longer necessary (Iben 1965, Wagoner, Fowler & Hoyle 1967) to approximate hard-won laboratory results on nuclear reaction rates by crude power-law dependences on temperature. In this article we review the available experimental data on cross sections for the nuclear interactions of neutrons, protons, and alpha particles with a number of light and intermediate-mass nuclei and we present calculations on the resulting reaction rates, nuclear lifetimes, and energy generation rates under astrophysical conditions. We restrict our considerations to nondegenerate, nonrelativistic circumstances for the interacting nuclei. Table I lists the general nuclear processes discussed, along with the units used in presenting numerical results and the notation used in representing nuclear reactions. Previous reviews of nuclear reaction rates, somewhat more limited in scope, have been given by Fowler (1954, 1960) , Burbidge, Burbidge, Fowler & Hoyle (1957) (hereafter referred to as B^2FH), Caughlan & Fowler (1962), and Parker, Bahcall & Fowler (1964). The last previous overall survey of nuclear reaction rates which has come to our attention is that of Reeves (1965).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1146/annurev.aa.05.090167.002521DOIArticle
http://www.annualreviews.org/doi/10.1146/annurev.aa.05.090167.002521PublisherArticle
Additional Information:© 1967 Annual Reviews. The survey of literature for this review was concluded in December 1966. Work supported in part by the Office of Naval Research [Nonr-220(47)] and the National Science Foundation [GP-5391] at the California Institute of Technology. Work supported in part by the National Science Foundation [GP-4693 and GP-6309] at Montana State University.
Funders:
Funding AgencyGrant Number
Office of Naval Research (ONR)Nonr-220(47)
NSFGP-5391
NSFGP-4693
NSFGP-6309
Record Number:CaltechAUTHORS:20161019-081138741
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20161019-081138741
Official Citation:Thermonuclear Reaction Rates William A. Fowler, Georgeanne R. Caughlan, and Barbara A. Zimmerman Annual Review of Astronomy and Astrophysics, Vol. 5: 525 -570 (Volume publication date September 1967)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:71254
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Oct 2016 16:17
Last Modified:19 Oct 2016 16:17

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