LEADER 05094nam 22006494a 450 001 9910828312803321 005 20200520144314.0 010 $a981-277-390-8 024 3 $a9789812567376 035 $a(CKB)1000000000410163 035 $a(EBL)1679797 035 $a(OCoLC)181590708 035 $a(SSID)ssj0000209884 035 $a(PQKBManifestationID)11198216 035 $a(PQKBTitleCode)TC0000209884 035 $a(PQKBWorkID)10265657 035 $a(PQKB)10527368 035 $a(MiAaPQ)EBC1679797 035 $a(EXLCZ)991000000000410163 100 $a20061003d2005 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aNeutrino physics $eproceedings of Nobel Symposium 129 : Haga Slott, Enkoping, Sweden, August 19-24, 2004 /$feditors, L. Bergstrom ... [et al.] 205 $a1st ed. 210 $aNew Jersey $cWorld Scientific$dc2005 215 $a1 online resource (192 p.) 225 1 $aPhysica scripta ;$vv. T121 300 $a"Recognised by the European Physical Society." 311 $a981-256-737-2 320 $aIncludes bibliographical references. 327 $aContents ; John N. Bahcall (1934-2005) ; Preface ; List of Participants ; Committees ; Nobel Symposium on Neutrino Physics-Program ; The History of Neutrino Oscillations ; 1. Introduction ; 2. B. Pontecorvo ; 3. Z. Maki M . Nakagawa and S. Sakata 327 $a4. B. Pontecorvo and collaborators 5. Conclusion ; References ; Super-Kamiokande Results on Neutrino Oscillations ; 1. Super-Kamiokande ; 2. Atmospheric neutrinos ; 3. Solar neutrinos ; 4. Super-Kamiokande II and III ; 5. Future of Super-Kamiokande ; References 327 $aSudbury Neutrino Observatory Results 1. Introduction ; 2. Resolving the solar neutrino ""Problem"" ; 3. The Sudbury Neutrino Observatory ; 4. SNO measurements to date ; 5. Future SNO and SNOLAB measurements ; References ; Results from KamLAND Reactor Neutrino Detection 327 $a1. Introduction 2. KamLAND detector ; 3. Detector performance ; 4. Reactor anti-neutrino detection ; 5. Data analysis ; 6. Neutrino oscillation analysis ; 7. Conclusions ; References ; New Opportunities for Surprise ; 1. Five clues and ideas ; 2. Why accelerator beams? 327 $a3. One example surprise: what if LSND is correct? 4. An example explanation: sterile neutrinos ; 5. Pursuing these questions: MiniBooNE and beyond ; 6. Conclusions ; References ; Solar Models and Solar Neutrinos ; 1. Introduction ; 2. Solar model fluxes 327 $a3. Recent developments regarding the solar surface composition 330 $aNobel Symposium 129 on Neutrino Physics was held at Haga Slott in Enko?ping, Sweden during August 19-24, 2004. Invited to the symposium were around 40 globally leading researchers in the field of neutrino physics, both experimental and theoretical. The dominant theme of the lectures was neutrino oscillations, which after several years were recently verified by results from the Super-Kamiokande detector in Kamioka, Japan and the SNO detector in Sudbury, Canada. Discussion focused especially on effects of neutrino oscillations derived from the presence of matter and the fact that three differen 410 0$aPhysica scripta (Stockholm, Sweden : 1982) ;$vv. T121. 606 $aNeutrinos$vCongresses 606 $aNeutrino interactions$vCongresses 606 $aSolar neutrinos$vCongresses 615 0$aNeutrinos 615 0$aNeutrino interactions 615 0$aSolar neutrinos 676 $a539.7/215 701 $aBergstrom$b L$g(Lars)$00 712 12$aNobel Symposium 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910828312803321 996 $aNeutrino physics$93976589 997 $aUNINA