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Record Nr. |
UNINA9910822038703321 |
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Autore |
Barger V (Vernon), <1938-> |
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Titolo |
The physics of neutrinos / / Vernon Barger, Danny Marfatia, Kerry Whisnant |
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Pubbl/distr/stampa |
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Princeton, : Princeton University Press, c2012 |
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ISBN |
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1-283-54007-X |
9786613852526 |
1-4008-4559-9 |
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Edizione |
[Course Book] |
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Descrizione fisica |
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1 online resource (239 p.) |
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Classificazione |
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Altri autori (Persone) |
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MarfatiaDanny <1972-> |
WhisnantKerry Lewis |
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Disciplina |
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Soggetti |
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Lingua di pubblicazione |
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Formato |
Materiale a stampa |
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Livello bibliografico |
Monografia |
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Note generali |
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Description based upon print version of record. |
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Nota di bibliografia |
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Includes bibliographical references and index. |
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Nota di contenuto |
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Front matter -- Contents -- Preface -- 1. Introduction -- 2. Neutrino Basics -- 3. Neutrino Mixing and Oscillations -- 4. Solar Neutrinos -- 5. Atmospheric Neutrinos -- 6. Global Three-neutrino Fits -- 7. Absolute Neutrino Mass -- 8. Long-baseline Neutrino Oscillations -- 9. Model Building -- 10. Supernova Neutrinos -- 11. High-energy Astrophysical Neutrinos -- 12. Beyond Three Neutrinos -- 13. Summary and Outlook -- References -- Index |
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Sommario/riassunto |
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The physics of neutrinos--uncharged elementary particles that are key to helping us better understand the nature of our universe--is one of the most exciting frontiers of modern science. This book provides a comprehensive overview of neutrino physics today and explores promising new avenues of inquiry that could lead to future breakthroughs. The Physics of Neutrinos begins with a concise history of the field and a tutorial on the fundamental properties of neutrinos, and goes on to discuss how the three neutrino types interchange identities as they propagate from their sources to detectors. The book shows how studies of neutrinos produced by such phenomena as cosmic rays in the atmosphere and nuclear reactions in the solar interior provide striking evidence that neutrinos have mass, and it traces our astounding progress in deciphering the baffling |
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