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                  | DATE: | 2012-12-07  16:00 - 17:00 |  
                  | PLACE: | Tsukuba Campus  building No.4  room#345 |  
                  | TITLE: | physics seminar / Reactor theta_13; the Ultimate Measurement? |  
                  | CONTACT: | Takasumi Maruyama |  
                  | SPEAKER: | Pau NOVELLA  (Marie Curie Fellow/CNRS-APC, Paris) |  
                  | LANGUAGE: | English |  
                  | ABSTRACT: | A new neutrino oscillation mode has been observed in around 2011-2012 by reactor neutrino experiments. This oscillation mode was expected under
 the 3 neutrino oscillations model characterised by the PMNS mixing
 leptonic flavour matrix , where the so-called "solar" and "atmospheric"
 modes are modulated by the the mixing angles ¦È12 and ¦È23, respectively.
 The new oscillation is modulated by ¦È13. Amazing progress has been
 obtained thanks to the precise contributions of the reactor neutrino
 experiments (alphabetically ordered: Daya Bay, Double Chooz, RENO).
 Consistent evidence towards ¦È13 oscillations had been obtained from
 electron neutrino appearance by T2K and MINOS experiments and the
 tension between combined Solar experiments and KamLAND results. sin^2(2¦È>13) is now known to be around 0.1 -as large as the CHOOZ limit allowed
 it to be- while the current precision is around 15%, dominated by the
 Daya Bay measurements. In this seminar, the global reactor ¦È13
 measurement situation will be reviewed. The final best reactor ¦È13
 measurement (full statistics envisaged by end of ~2015) will dominate
 our knowledge on this parameter for a long time. No other technique,
 with current technologies, is expected to offer cleaner input on the
 value of ¦È13. We will cover discussion on the experimental progress to
 ensure a precise but also the most accurate measurement of ¦È13. The
 impact of the accuracy on the knowledge of ¦È13 will be highlighted
 within the phenomenological context of a coherent 3-neutrino oscillation
 model.
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