Published May 20, 1968
| Published
Journal Article
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Present Status of the Theoretical Predictions for the ^(37)Cl Solar-Neutrino Experiment
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.Attached Files
Published - BAHprl68.pdf
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Additional details
- Alternative title
- Present Status of the Theoretical Predictions for the ^(36)Cl Solar-Neutrino Experiment
- Eprint ID
- 33199
- Resolver ID
- CaltechAUTHORS:20120815-093355459
- GP-7976
- NSF
- Nonr-220(47)
- Office of Naval Research (ONR)
- Alfred P. Sloan Foundation Fellowship
- GP-6928
- NSF
- GP-5391
- NSF
- Created
-
2012-08-15Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field