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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