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Solar neutrinos, oscillations, and mixing

Author: Wick C Haxton; University of California, Berkeley. Department of Physics.
Publisher: 1997.
Edition/Format:   VHS video : VHS tape   Visual material : English
Database:WorldCat
Summary:
A lecture by Professor Wick Haxton of the University of Washington, Seattle on the "solar neutrino problem": The discrepancy between the predictions of the standard solar model and the results of the chlorine, Kamioka, and SAGE/GALLEX experiments is often considered strong evidence for new particle physics. Indeed, the solar enhancement of neutrino oscillations, a phenomenon that has familiar analogs in coupled  Read more...
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Genre/Form: Congresses
Material Type: Videorecording
Document Type: Visual material
All Authors / Contributors: Wick C Haxton; University of California, Berkeley. Department of Physics.
OCLC Number: 37178601
Event notes: Recorded at a colloquium held on April 28, 1997, sponsored by the Dept. of Physics, University of California, Berkeley.
Description: 1 videocassette : sd., color ; 1/2 in.
Details: VHS.
Responsibility: Wick Haxton.

Abstract:

A lecture by Professor Wick Haxton of the University of Washington, Seattle on the "solar neutrino problem": The discrepancy between the predictions of the standard solar model and the results of the chlorine, Kamioka, and SAGE/GALLEX experiments is often considered strong evidence for new particle physics. Indeed, the solar enhancement of neutrino oscillations, a phenomenon that has familiar analogs in coupled pendula, provides a plausible explanation for the measurements. Yet, despite claims to the contrary, he argues that nonstandard solar model solutions are not yet ruled out. He discusses how experiments currently underway might be augmented to provide more constraints on proposed solutions.

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