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Importance of a study of the decay of Ca^(37) to the problem of detecting solar neutrinos

Bahcall, J. N. and Barnes, C. A. (1964) Importance of a study of the decay of Ca^(37) to the problem of detecting solar neutrinos. Physics Letters, 12 (1). pp. 48-49. ISSN 0031-9163. https://resolver.caltech.edu/CaltechAUTHORS:20150908-150519805

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Abstract

Recent theoretical and experimental work has shown that a direct test of the theory of stellar energy generation in main sequence stars is possible by detecting solar neutrinos with the reaction Cl^(37) + ^v_(solar) → A^(37) e^-. In order to relate the counting rate in the proposed experiment to the flux of solar neutrinos (and thus ultimately to parameters describing the interior of the sun), one must know the matrix elements for neutrino capture to all the relevant states in A^(37).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/0031-9163(64)91171-0DOIArticle
http://www.sciencedirect.com/science/article/pii/0031916364911710PublisherArticle
Additional Information:© 1964 Published by Elsevier B.V. Received 5 August 1964. Available online 1 October 2002. Supported in part by the Office of Naval Research and the National Aeronautics and Space Administration.
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Funding AgencyGrant Number
Office of Naval Research (ONR)UNSPECIFIED
NASAUNSPECIFIED
Issue or Number:1
Record Number:CaltechAUTHORS:20150908-150519805
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150908-150519805
Official Citation:Importance of a study of the decay of Ca37 to the problem of detecting solar neutrinos J.N. Bahcall, C.A. Barnes Volume 12, Issue 1, 1 September 1964, Pages 48-49
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:60100
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:09 Sep 2015 19:32
Last Modified:03 Oct 2019 08:53

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