Neutrino Physics: Proceedings of Nobel Symposium 129 9789812567376, 9812567372, 9189621271

Table of contents :
Contents......Page 4
John N. Bahcall (1934-2005)......Page 8
Preface......Page 10
List of Participants......Page 12
Committees......Page 14
Nobel Symposium on Neutrino Physics-Program......Page 15
1. Introduction......Page 18
2. B. Pontecorvo......Page 19
4. B. Pontecorvo and collaborators......Page 20
References......Page 22
2. Atmospheric neutrinos......Page 24
3. Solar neutrinos......Page 27
References......Page 29
2. Resolving the solar neutrino "Problem"......Page 30
4. SNO measurements to date......Page 31
References......Page 33
2. KamLAND detector......Page 34
4. Reactor anti-neutrino detection......Page 35
5. Data analysis......Page 36
6. Neutrino oscillation analysis......Page 38
References......Page 39
2. Why accelerator beams?......Page 40
3. One example surprise: what if LSND is correct?......Page 41
4. An example explanation: sterile neutrinos......Page 42
5. Pursuing these questions: MiniBooNE and beyond......Page 43
References......Page 45
2. Solar model fluxes......Page 47
4. Neutrinos as dark matter......Page 50
References......Page 51
1. Introduction......Page 52
2. Calculation......Page 53
3. Higher energies......Page 54
References......Page 56
2. The MSW effect......Page 58
3. Realizations of the MSW effect......Page 60
4. Matter effects in neutrino oscillations......Page 62
References......Page 64
2. Leptonic mixing and neutrino oscillations......Page 66
5. 3f effects in neutrino oscillations......Page 67
7. CP- and T-odd effects in v oscillations in matter......Page 70
8. Why study Ue3? (A hymn to Ue3)......Page 71
References......Page 72
1. Introduction: the New Minimal Standard Model......Page 73
2. Orthodox fits......Page 74
3. Unorthodox fits......Page 77
References......Page 78
2. Three neutrino oscillation in matter......Page 79
3. Correlations and degeneracies......Page 81
4. The potential of future neutrino oscillation experiments......Page 82
5. Theoretical implications and conclusions......Page 85
References......Page 86
1. Introduction......Page 87
3. Present experimental results......Page 88
4. The future......Page 91
5. Conclusions......Page 92
References......Page 94
2. The neutrino mixing parameters and (BB)0v -decay......Page 95
3. Properties of Majorana neutrinos: brief summary......Page 98
4. Predictions for the effective Majorana mass......Page 99
5. Implications of measuring |(m)| = 0......Page 100
References......Page 101
2. Core-collapse Supernovae as neutrino sources......Page 103
4. Experimental signatures......Page 104
References......Page 105
1. Neutrinos associated with the highest energy cosmic rays......Page 107
3. Neutrino telescopes: first "Light"......Page 109
4. Mediterranean telescopes......Page 110
5. Kilometer-scale neutrino observatories......Page 111
References......Page 112
2. Design of NT-200 and AMANDA......Page 113
3. Physics results from NT-200 and AMANDA......Page 114
4. IceCube......Page 118
References......Page 119
1. Cosmic neutrinos for astrophysicists and particle physicists......Page 120
2. Quantifying cosmic neutrino detection......Page 121
3. Radio detection......Page 122
5. Other neutrino telescope techniques......Page 124
References......Page 125
2. Sources of very high energy neutrinos......Page 127
3. Methods of detecting high energy neutrinos using extensive air showers......Page 128
References......Page 130
2. The standard relic neutrino background......Page 132
3. Non-Standard neutrino backgrounds......Page 133
6. Prospects for laboratory searches: effects linear in GF......Page 134
References......Page 136
1. Introduction......Page 138
2. Thermal leptogenesis......Page 139
3. Nonthermal leptogenesis via inflaton decay......Page 140
4. Conclusions......Page 141
References......Page 142
2. Notation......Page 143
3. CBR......Page 144
4. BBN......Page 145
5. CBR and BBN combined......Page 146
References......Page 147
1. Introduction and summary......Page 148
2. Phenomenological considerations......Page 149
References......Page 152
2. The physics underlying cosmological neutrino bounds......Page 154
3. What are the constraints?......Page 155
References......Page 156
2. The neutrino-antineutrino relation......Page 157
3. Consequences of Majorana character......Page 159
4. A concluding question......Page 160
References......Page 161
1 Introduction......Page 162
3. The NuTeV neutrino experiment......Page 163
4. Interpretations of the NuTeV result......Page 164
5. Future measurements......Page 165
References......Page 166
1. Introduction......Page 167
2. Direct neutrino mass experiments......Page 168
3. The KATRIN experiment......Page 170
References......Page 172
2. The data......Page 173
4. A pinch of Grand Unification......Page 174
6. Beyond Froggatt-Nielsen......Page 175
7. Cabibbo flop......Page 176
References......Page 177
2. See-saw mechanism......Page 179
5. Mixing angles from the charged leptons?......Page 180
6. Phenomenological implications......Page 181
7. Model building applications......Page 182
8. Leptogenesis......Page 183
References......Page 184
1. Introduction......Page 186
2. Seesaw mechanism B-L and left-right symmetry......Page 187
3. Seesaw and large neutrino mixings......Page 188
4. A predictive minimal SO(10) theory for neutrinos......Page 189
6. Quark-lepton complementarity and large solar mixing......Page 191
References......Page 192