Probing the neutrino mass hierarchy with Super-Kamiokande

被引：6

作者：

Agarwalla, Sanjib Kumar ^{[1
]}

Hernandez, Pilar ^{[1
]}

机构：

[1] Univ Valencia, CSIC, Inst Fis Corpuscular, E-46071 Valencia, Spain

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2012年 / 10期

关键词：

Neutrino Physics; Beyond Standard Model; MAGIC BASE-LINE; OSCILLATION PARAMETERS; MATTER; RESONANCE; DECAY;

D O I：

10.1007/JHEP10(2012)086

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We show that for recently discovered large values of theta(13), a superbeam with an average neutrino energy of similar to 5 GeV, such as those being proposed at CERN, if pointing to Super-Kamiokande (L similar or equal to 8770 km), could reveal the neutrino mass hierarchy at 5 sigma in less than two years irrespective of the true hierarchy and CP phase. The measurement relies on the near resonant matter effect in the nu(mu) -> nu(e) oscillation channel, and can be done counting the total number of appearance events with just a neutrino beam.

引用

页数：14

共 50 条

[31] Super-Kamiokande data and atmospheric neutrino decay
Fogli, GL
Lisi, E
Marrone, A
Scioscia, G
PHYSICAL REVIEW D, 1999, 59 (11):
[32] Establishing atmospheric neutrino oscillations with Super-Kamiokande
Kajita, T.
Kearns, E.
Shiozawa, M.
NUCLEAR PHYSICS B, 2016, 908 : 14 - 29
[33] Solar neutrino measurement in Super-Kamiokande III
Ikeda, M.
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2011, 217 : 124 - 126
[34] Solar neutrino results from Super-Kamiokande
Takeuchi, Y
INTERNATIONAL JOURNAL OF MODERN PHYSICS A, 2003, 18 (22): : 3777 - 3787
[35] Supernova relic neutrino search at super-Kamiokande
Bays, K.
Iida, T.
Abe, K.
Hayato, Y.
Iyogi, K.
Kameda, J.
Koshio, Y.
Marti, L.
Miura, M.
Moriyama, S.
Nakahata, M.
Nakayama, S.
Obayashi, Y.
Sekiya, H.
Shiozawa, M.
Suzuki, Y.
Takeda, A.
Takenaga, Y.
Ueno, K.
Ueshima, K.
Yamada, S.
Yokozawa, T.
Kaji, H.
Kajita, T.
Kaneyuki, K.
McLachlan, T.
Okumura, K.
Lee, K. P.
Martens, K.
Vagins, M.
Labarga, L.
Kearns, E.
Litos, M.
Raaf, J. L.
Stone, J. L.
Sulak, L. R.
Kropp, W. R.
Mine, S.
Regis, C.
Renshaw, A.
Smy, M. B.
Sobel, H. W.
Ganezer, K. S.
Hill, J.
Keig, W. E.
Cho, S.
Jang, J. S.
Kim, J. Y.
Lim, I. T.
Albert, J.
PHYSICAL REVIEW D, 2012, 85 (05):
[36] Low Energy Neutrino Physics at Super-Kamiokande
Smy, Michael B.
TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP2009), 2010, 203
[37] Kamiokande and super-kamiokande
Suzuki, Y
PROGRESS IN PARTICLE AND NUCLEAR PHYSICS, VOL 40: NEUTRINOS IN ASTRO, PARTICLE AND NUCLEAR PHYSICS, 1998, 40 : 427 - 441
[38] Solar neutrino results from Super-Kamiokande
Suzuki, Y
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 2001, 91 : 29 - 35
[39] Kamiokande and Super-Kamiokande
Univ of Tokyo, Gifu, Japan
Progr Part Nucl Phys, (427-441):
[40] Solar neutrino results from Super-Kamiokande
Suzuki, Y
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 1999, 77 : 35 - 42

← 1 2 3 4 5 →