LEADER 05402nam 22006614a 450 001 9910453191703321 005 20200520144314.0 010 $a1-281-91186-0 010 $a9786611911867 010 $a981-277-197-2 035 $a(CKB)1000000000538171 035 $a(EBL)1681390 035 $a(OCoLC)879025099 035 $a(SSID)ssj0000209882 035 $a(PQKBManifestationID)11198215 035 $a(PQKBTitleCode)TC0000209882 035 $a(PQKBWorkID)10266351 035 $a(PQKB)11130865 035 $a(MiAaPQ)EBC1681390 035 $a(WSP)00002053 035 $a(Au-PeEL)EBL1681390 035 $a(CaPaEBR)ebr10255475 035 $a(CaONFJC)MIL191186 035 $a(EXLCZ)991000000000538171 100 $a20080716d2008 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 00$aNeutrino oscillations$b[electronic resource] $epresent status and future plans /$feditors, Jennifer A. Thomas, Patricia L. Vahle 210 $a[Singapore] ;$aNew Jersey $cWorld Scientific$dc2008 215 $a1 online resource (274 p.) 300 $aDescription based upon print version of record. 311 $a981-277-196-4 320 $aIncludes bibliographical references and indexes. 327 $aContents; Preface; 1. Neutrino Oscillation Phenomenology S. J. Parke; 1.1. Introduction; 1.2. The ?e Disappearance Channel; 1.2.1. Reactor Experiments at the Solar L/E; 1.2.2. Reactor Experiments at the Atmospheric L/E; 1.2.3. Solar Neutrinos; 1.3. The ??????? Disappearance Channel; 1.4. The Appearance Channel; 1.5. Beyond the Neutrino Mixing Model; 1.6. Summary and Conclusion; Acknowledgments; References; 2. The Super-Kamiokande Experiment C. W. Walter; 2.1. Introduction and Physics Goals; 2.2. The Super-Kamiokande Detector; 2.3. Published Results from Super-Kamiokande 327 $a2.3.1. Atmospheric Neutrino Oscillations2.3.2. Solar Neutrino Oscillations; 2.3.3. The Search for Proton Decay; 2.3.4. The Search for Astrophysical Phenomenon; 2.4. Conclusions; Acknowledgments; References; 3. Sudbury Neutrino Observatory S. J. M. Peeters and J. R. Wilson; 3.1. Introduction; 3.2. The SNO Detector; 3.2.1. Signals; 3.2.2. Calibration; 3.2.3. Backgrounds; 3.3. Analysis Strategy; 3.3.1. Signal Extraction; 3.3.1.1. Flux Calculations; 3.3.1.2. Spectrum Measurement; 3.3.1.3. Day-Night Neutrino Flux Asymmetry; 3.4. Phase 1 D2O; 3.5. Phase 2 Salt 327 $a3.6. Phase 3 Neutral Current Detection Array3.6.1. The Counter System; 3.6.2. The Backgrounds; 3.6.3. The Installation of the NCD System; 3.6.4. Data-Taking Period; 3.7. Conclusions; Acknowledgments; References; 4. Neutrino Oscillation Physics with KamLAND: Reactor Antineutrinos and Beyond K. M. Heeger; 4.1. Neutrino Physics at Reactors: From the Discovery of ?e to Nuclear Non-Proliferation; 4.2. The KamLAND Detector; 4.2.1. Observation of Reactor Antineutrino Disappearance; 4.3. Spectral Distortion as a Signature of Neutrino Oscillation; 4.4. Toward a Precision Measurement of m2 12 and ?12 327 $a4.5. Other Neutrino Physics with KamLAND4.6. Test of MSW and Non-Standard Interactions in the KamLAND Low-Background Phase; 4.7. Summary and Conclusions; Acknowledgments; References; 5. K2K: KEK to Kamioka Long-Baseline Neutrino Oscillation Experiment R. J. Wilkes; 5.1. Introduction; 5.2. Neutrino Beam; 5.3. Beam Simulation; 5.4. The Near Detectors; 5.5. The Far Detector; 5.6. Neutrino Interaction Simulations; 5.7. Event Rates and Oscillation Analysis; 5.8. Summary and Conclusions; Acknowledgments; References; 6. MINOS P. Vahle; 6.1. Introduction; 6.2. The NuMI Beam; 6.3. The MINOS Detectors 327 $a6.4. Calibration6.5. Event Selection; 6.6. Near Detector Data and Monte Carlo; 6.7. Predicting the Far Detector Spectrum; 6.8. Systematics; 6.9. Results; 6.10. Outlook; Acknowledgments; References; 7. The LSND and KARMEN Neutrino Oscillation Experiments W. C. Louis; 7.1. Introduction; 7.2. LSND; 7.2.1. Description of the Experiment; 7.2.2. Event Selection; 7.2.3. Neutrino Oscillation Signal and Background Reactions; 7.2.4. Neutrino Oscillation Results; 7.3. KARMEN; 7.3.1. Description of the Experiment; 7.3.2. Event Selection; 7.3.3. Neutrino Oscillation Signal and Background Reactions 327 $a7.3.4. Neutrino Oscillation Results 330 $a This book reviews the status of a very exciting field - neutrino oscillations - at a very important time. The fact that neutrinos have mass has only been proved in the last few years and the acceptance of that fact has opened up a whole new area of study to understand the fundamental parameters of the mixing matrix. The book summarizes the results from all the experiments which have played a role in the measurement of neutrino oscillations and briefly describes the scope of some new planned experiments. Contributions include a theoretical introduction by Stephen Parke from FNAL, as well as a 606 $aNeutrinos 606 $aOscillations 608 $aElectronic books. 615 0$aNeutrinos. 615 0$aOscillations. 676 $a539.7/215 701 $aThomas$b Jennifer A$0936164 701 $aVahle$b Patricia L$0936165 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910453191703321 996 $aNeutrino oscillations$92108892 997 $aUNINA LEADER 01538nam 2200337 n 450 001 996390873903316 005 20200824121828.0 035 $a(CKB)4940000000107047 035 $a(EEBO)2240902291 035 $a(UnM)99861036e 035 $a(UnM)99861036 035 $a(EXLCZ)994940000000107047 100 $a19920106d1645 uh | 101 0 $aeng 135 $aurbn||||a|bb| 200 13$aAn ordinance of the Lords and Commons assembled in Parliament$b[electronic resource] $efor the more effectuall puting in execution the Directory for publique worship, in all parish churches and chappells within the kingdome of England and dominion of Wales, and for the dispersing of them in all places and parishes within this kindome [sic], and the dominion of Wales. Ordered by the Commons in Parliament, that this ordinance be forthwith printed and published: H. Elsynge, Cler. Parl. D. Com 210 $a[London] $cPrinted by T.W. for Ed. Husband, printer for the Honourable House of Commons.$d1645 215 $a[2], 6 p 300 $aPlace of publication from Wing. 300 $aAnnotation on Thomason copy: "Aug: 25". 300 $aReproduction of the original in the British Library. 330 $aeebo-0018 607 $aGreat Britain$xReligion$y17th century$vEarly works to 1800 801 0$bCu-RivES 801 1$bCu-RivES 801 2$bCStRLIN 801 2$bWaOLN 906 $aBOOK 912 $a996390873903316 996 $aAn ordinance of the Lords and Commons assembled in Parliament$92298865 997 $aUNISA