Published October 14, 1991
| public
Journal Article
The reaction branching ^(31)P(p, γ)/^(31)P(p, α) in the RP-process
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.
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.Additional details
- Eprint ID
- 60258
- Resolver ID
- CaltechAUTHORS:20150915-133355526
- PHY88-03035
- NSF
- PHY88-17296
- NSF
- Natural Sciences and Engineering Research Council of Canada (NSERC)
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2015-09-15Created from EPrint's datestamp field
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2021-11-10Created from EPrint's last_modified field