Analysis of neutrino oscillation in three-flavor neutrinos

被引：21

作者：

Sakai, T ^{[1
]}

Inagaki, O ^{[1
]}

Teshima, T ^{[1
]}

机构：

[1] Chubu Univ, Dept Appl Phys, Kasugai, Aichi 4878501, Japan

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 1999年 / 14卷 / 12期

关键词：

D O I：

10.1142/S0217751X99000981

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

We analyze the solar, terrestrial and atmospheric neutrino experiments including Super-Kamiokande data using the three-flavor neutrinos framework and obtain the allowed region for parameters (Delta m(12)(2), sin(2) 2 theta(12), Delta m(23)(2), theta(13), theta(23)). In solar neutrino experiments, we obtain the large angle solution (Delta m(12)(2), sin(2) 2 theta(12)) = (4x10(-6) -7x10(-5) eV(2), 0.6-0.9) and small angle solution (3 x 10(-6) - 1.2 x 10(-5) eV(2), 0.003 - 0.01) for theta(13) = 0 degrees - 20 degrees. From the terrestrial and atmospheric neutrino experiments including the sub-GeV and multi-GeV zenith angle dependence in SuperKamiokande 535 days data, we found that the nu(mu)- nu(tau) mixing is large and the range of Delta m(23)(2) as 0.02 similar to 0.0002 eV(2). There is no significant difference between large theta(12) angle solution and small one.

引用

页码：1953 / 1974

页数：22

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