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Prospects of reactor neutrino experiments

โœ Scribed by F. Suekane


Publisher
Elsevier Science
Year
2010
Tongue
English
Weight
564 KB
Volume
64
Category
Article
ISSN
0146-6410

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โœฆ Synopsis


Mass hierarchy a b s t r a c t

Since the energy of a reactor neutrino is a few MeV, all m 2 12 , m 2 23 and m 2 13 oscillations are accessible by reactor neutrino experiments. KamLAND observed the m 2 12 oscillation and currently Double Chooz, RENO and Dayabay experiments are under construction aiming to detect m 2 13 + m 2 23 oscillation. There are still good prospects for future reactor neutrino experiments after them. For example, there is room to further improve sin 2 2ฮธ 13 accuracy at a baseline of โˆผ1.5 km, a very precise sin 2 2ฮธ 12 measurement and the determination of mass hierarchy may be possible at a baseline โˆผ50 km, and if KamLAND is enlarged to the SuperKamiokande size, better measurement of m 2 12 and sin 2 2ฮธ 12 will be anticipated. It is important to take into account such possibilities when planning future neutrino program after ฮธ 13 is measured by current experiments.


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