Solar neutrinos : the first thirty years
著者
書誌事項
Solar neutrinos : the first thirty years
（Frontiers in physics, v. 92）
Addison-Wesley, the Advanced Book Program, 1995
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注記
Includes bibliographical references
内容説明・目次
内容説明
The papers reprinted in this book depict a research field that is poised to answer some of the fundamental questions of twentieth-century physics and astronomy: How does the sun shine? What is the dark matter? Is there new physics beyond the standard model?. }The papers reprinted in this book depict a research field that is poised to answer some of the fundamental questions of twentieth-century physics and astronomy: How does the sun shine? What is the dark matter? Is there new physics beyond the standard model?This book is of interest to students as well as active researchers in the scientific areas spanned by the reprinted papers, which include physics, chemistry, astronomy, geology, and engineering. Historians of science, some of whom have already used the solar neutrino problem as a case study, will also find this collection a rich source of examples and insights. Solar Neutrinos gives on the special feeling of being present at the birth of a scientific field. The physical ideas are presented with a simplicity that is unusual in review of papers.
By delving into the scientific landmarks reprinted here, one can see clearly how researchers-starting with a paucity of data and with conflicting hypothesis-struggled together to grope their way to a better understanding of the sun and of weak interaction physics. }
目次
- Standard Model Expectations
- Introduction (John N. Bahcall)
- Neutrino Cross Sections
- Early Solar Models
- Sensitivity Studies
- Refined Solar Models
- Solar Neutrino Experiments
- First Proposals of Experiments Now Being Performed
- Initial Experimental Results
- Other Proposed Experiments
- Nuclear Fusion Reactions
- Introduction (Peter Parker)
- Exploratory Studies of Alternate Terminations
- Early Systematic Studies
- Recent Precision Studies
- Physics Beyond the Standard Model
- Vacuum Oscillations
- Neutrino Decay
- Neutrino Oscillations in Matter, Resonant Flavor Conversion
- Neutrino Spin-Flip Phenomena
- Flavor Mixing by New Interactions
- Helioseismology.
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