Neutrino Physics and Astrophysics
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Table of contents
- Cover
- Contentsviii
- Forewordiv
- International Neutrino Committeev
- Neutrino 98 International Advisory Committee/Organizing Committeevi
- Part 1: Opening Lecture1
- Chapter 1. Neutrinos: a glimpse beyond the Standard Model3
- Part 2: Solar Neutrinos11
- Chapter 2. The Homestake solar neutrino program13
- Chapter 3. Solar neutrino results from SAGE20
- Chapter 4. GALLEX solar neutrino results and status of GNO26
- Chapter 5. Solar neutrino results from Super-Kamiokande35
- Chapter 6. The Sudbury Neutrino Observatory project43
- Chapter 7. Status of the BOREXINO solar neutrino experiment48
- Chapter 8. Future solar neutrino projects55
- Chapter 9. Standard solar models64
- Chapter 10. Uncertainties in the solar neutrino flux73
- Chapter 11. Helioseismology and solar neutrinos81
- Chapter 12. Neutrino magnetic moment and solar neutrino experiments89
- Chapter 13. New enhancement mechanism of the transitions in the Earth of the solar and atmospheric n93
- Chapter 14. Towards the solution of the solar neutrino problem98
- Part 3: Atmospheric Neutrinos109
- Chapter 15. Atmospheric neutrino studies in Soudan 2111
- Chapter 16. Atmospheric neutrino induced muons in the MACRO detector117
- Chapter 17. Atmospheric neutrino results from Super-Kamiokande and Kamiokande - Evidence for vμ , o123
- Chapter 18. Fluxes of atmospheric neutrinos and related cosmic rays133
- Chapter 19. Uncertainty of the atmospheric neutrino fluxes140
- Chapter 20. vμ ↔v r vs vμ↔vs solutions for the atmospheric neutrino problem146
- Chapter 21. On the neutrino mass spectrum and neutrino mixing from oscillation data151
- Part 4: Long Baseline Experiments157
- Chapter 22. Results from CHOOZ159
- Chapter 23. The Palo Verde reactor neutrino oscillation experiment166
- Chapter 24. Present Status of KamLAND171
- Chapter 25. A pilot experiment with reactor neutrinos in Taiwan177
- Chapter 26. Long baseline neutrino oscillation program in the United States182
- Chapter 27. Physics projects for a future CERN-LNGS neutrino programme187
- Chapter 28. Status of K2K (KEK to Kamioka long baseline neutrino oscillation experiment)198
- Part 5: Short Baseline Oscillation Experiments205
- Chapter 29. Neutrino oscillation results from LSND207
- Chapter 30. The search for neutrino oscillations vμ->ve with KARMEN212
- Chapter 31. CHORUS results220
- Chapter 32. A search for vμ↔ vr Oscillations Using the NOMAD Detector225
- Chapter 33. Future short baseline neutrino oscillation experiments232
- Part 6: Implications of the Solar and Atmospheric Neutrino Data239
- Chapter 34. Implications of solar and atmospheric neutrinos241
- Part 7: Accelerator and Reactor Neutrino Experiments257
- Chapter 35. Result from DONUT- Direct observation of vt interaction-259
- Chapter 36. Determination of sin2 θw from neutrino-nucleon scattering at NuTeV265
- Chapter 37. Events with isolated charged leptons and missing momentum observed at the e+p collider H271
- Chapter 38. Neutrino physics with a muon collider276
- Chapter 39. Status of the MUNU experiment285
- Part 8: Neutrino and Particle Physics291
- Chapter 40. Large lepton mixing in seesaw models- Coset-space family unification293
- Chapter 41. Implications of the SuperKamiokande result on the nature of new physics299
- Chapter 42. Implications of a minimal SO(10) Higgs structure308
- Chapter 43. Cosmic ray and neutrino tests of special relativity313
- Part 9: Direct Search for Neutrino Mass319
- Chapter 44. New results from the Mainz neutrino mass experiment321
- Chapter 45. Neutrino mass and anomaly in the tritium beta-spectrum. Results of the "Troitsk v-mass"327
- Part 10: Double Beta Decay333
- Chapter 46. Review on double beta decay experiments and comparison with theory335
- Chapter 47. Double beta decays and neutrino nuclear responses346
- Chapter 48. Results from the NEMO experiment352
- Chapter 49. Double beta decay with Ge-detectors - and the future of double beta and dark matter sear357
- Chapter 50. Present and future of low temperature detectors369
- Chapter 51. Particle physics implications of neutrinoless double beta decay376
- Part 11: Dark Matter Search387
- Chapter 52. Direct searches for dark matter389
- Chapter 53. Indirect searches for dark matter398
- Chapter 54. Baryonic dark matter402
- Chapter 55. Theoretical overview: emphasis on neutrinos420
- Part 12: Neutrino in Cosmology and Astrophysics427
- Chapter 56. Supernova neutrinos: review429
- Chapter 57. Future supernova neutrino detection435
- Chapter 58. Pulsar velocities without neutrino mass440
- Chapter 59. The neutrino ground state in a neutron star445
- Chapter 60. Neutrino mass and baryon asymmetry450
- Chapter 61. Axion hunting at the turn of the millenium456
- Part 13: Ultra-high energy neutrinos463
- Chapter 62. High energy neutrino astrophysics465
- Chapter 63. The AMANDA neutrino telescope474
- Chapter 64. The Lake Baikal experiment486
- Chapter 65. Neutrino telescopes under the ocean: The case for ANTARES492
- Chapter 66. Extremely high energy cosmic rays and neutrinos498
- Part 14: Concluslon509
- Chapter 67. Beyond the Standard Model: this time for real511
- Chapter 68. Comments520
- Chapter 69. Concluding Words525
- List of Contribution Papers527
- List of Poster Presentations529
- List of Participants531
- Author Index543
- General Information547
The scientific program of these important proceedings was arranged to cover most of the field of neutrino physics. In light of the rapid growth of interest stimulated by new interesting results from the field, more than half of the papers presented here are related to the neutrino mass and oscillations, including atmospheric and solar neutrino studies. Neutrino mass and oscillations could imply the existence of a mass scale many orders of magnitudes higher than presented in current physics and will probably guide scientists beyond the standard model of particle physics.