CaltechAUTHORS
Published May 20, 1968 | Version Published
Journal Article Open

Present Status of the Theoretical Predictions for the ^(37)Cl Solar-Neutrino Experiment

Creators

Abstract

The theoretical predictions for the ^(37)Cl solar-neutrino experiment are summarized and compared with the experimental results of Davis, Harmer, and Hoffman. Three important conclusions about the sun are shown to follow.

Additional Information

© 1968 The American Physical Society. Received 8 April 1968. Supported in part by the National Science Foundation [GP-7976, formerly GP-5391] and the Office of Naval Research [Nonr-220(47)]. Alfred P. Sloan Foundation Fellow. Also at Tel Aviv University, Tel Aviv, Israel. Also supported by the National Science Foundation [GP-6928] with Cornell University. We are grateful to R. Davis, Jr., R. P. Feynman, William A. Fowler, P. Goldreich, D. L. Lambert, R. M. May, and F. Reines for stimulating and informative conversations, and to J. N. Stewart and A. N. Cox for supplying us with opacity tables for the Lambert-Warner solar composition.

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Additional details

Additional titles

Alternative title
Present Status of the Theoretical Predictions for the ^(36)Cl Solar-Neutrino Experiment

Identifiers

Eprint ID
33199
Resolver ID
CaltechAUTHORS:20120815-093355459

Funding

NSF
GP-7976
Office of Naval Research (ONR)
Nonr-220(47)
Alfred P. Sloan Foundation Fellowship
NSF
GP-6928
NSF
GP-5391

Dates

Created
2012-08-15
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Updated
2021-11-09
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