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The reaction branching ^(31)P(p, γ)/^(31)P(p, α) in the RP-process

Iliadis, C. and Giesen, U. and Görres, J. and Graff, S. and Wiescher, M. and Azuma, R. E. and King, J. and Buckby, M. and Barnes, C. A. and Wang, T. R. (1991) The reaction branching ^(31)P(p, γ)/^(31)P(p, α) in the RP-process. Nuclear Physics A, 533 (1). pp. 153-169. ISSN 0375-9474. https://resolver.caltech.edu/CaltechAUTHORS:20150915-133355526

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Abstract

The reactions ^(31)P(p, γ)^(32)S and ^(31)P(p, α)^(28)Si have been studied in the energy range 280–620 keV to investigate the influence of low-energy resonances on the stellar reaction rates. Several new resonances have been observed and the resonance strengths for both reaction channels have been determined. The reaction rates have been calculated from the present results and are compared with the results of Hauser-Feshbach calculations.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/0375-9474(91)90824-PDOIArticle
http://www.sciencedirect.com/science/article/pii/037594749190824PPublisherArticle
Additional Information:© 1991 Elsevier. Received 12 March 1991. Revised 7 May 1991. This work was supported by the National Science Foundation Grants PHY88-03035 (Notre Dame), PHY88-17296 (Caltech} and by the Natural Science and Engineering Research Council of Canada. The authors wish to express their sincere gratitude to L. Curtis and the technical staff at the 350 keY accelerator of the University of Toledo, who made the implantation of the ^(31) P target possible.
Funders:
Funding AgencyGrant Number
NSFPHY88-03035
NSFPHY88-17296
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Subject Keywords:Nuclear reactions
Issue or Number:1
Record Number:CaltechAUTHORS:20150915-133355526
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150915-133355526
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:60258
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:15 Sep 2015 23:09
Last Modified:03 Oct 2019 08:55

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