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Future Prospects of KamLAND & q 13

sin 2 2 q may be shown to <1??. (No official plot. Just to get a sense.). 2005 fall: 4 p calibration ( s fid : 4.7%->3%). error (%). KL-II:. Solar 7 Be n. Future Prospects of KamLAND & q 13. KL is still only long baseline reactor n experiment in near future. KL-III:.

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Future Prospects of KamLAND & q 13

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  1. sin22q may be shown to <1?? (No official plot. Just to get a sense.) 2005 fall: 4p calibration (sfid: 4.7%->3%) error (%) KL-II: Solar 7Be n Future Prospects of KamLAND & q13 KL is still only long baseline reactor n experiment in near future KL-III: Large mass and very low BG environment may be suitable for bb battle field???

  2. q13: a key to the future * Detectability of CPV d: depends on q13 Large q13 OK, Let's proceed to CPV experiments Small q13 ummm... Solar Atmospheric Reactor Long baseline d: unknown

  3. Near Future q13 measurements sin22q23=0.95 matter effect ignored Accelerator Measurement sin2q23=0.61 sin2q23=0.39 P(nm->ne) ICARUS(Europe) MINOS(USA) NOVA(USA) OPERA(Europe) T2K(Japan) sin22q13 Reactor Measurement Cooperation of Accelerator + Reactor Necessary to resolve ambiguity and perform precision measurement Angra (Brasil) ,Braidwood (USA), DayaBay (China),DCHOOZ (French), KASKA (Japan), RENO(Korea)

  4. 2005 2008 Reactor1.5 2009 Near Future Prospect ~2007 sin22q13~0.06 ~2010 sin22q13~0.03 ~2012 sin22q13~0.02 ~2015 sin22q13~0.01 P.Huber et. al. hep-ph/0412133v1 will see if or

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