CONSTRAINTS ON NEUTRINO-OSCILLATION PARAMETERS FROM THE KAMIOKANDE-II SOLAR-NEUTRINO DATA

被引：146

作者：

HIRATA, KS

INOUE, K

KAJITA, T

KIFUNE, T

KIHARA, K

NAKAHATA, M

NAKAMURA, K

OHARA, S

SATO, N

SUZUKI, Y

TOTSUKA, Y

YAGINUMA, Y

MORI, M

OYAMA, Y

SUZUKI, A

TAKAHASHI, K

YAMADA, M

KOSHIBA, M

SUDA, T

TAJIMA, T

MIYANO, K

MIYATA, H

TAKEI, H

FUKUDA, Y

KODERA, E

NAGASHIMA, Y

TAKITA, M

KANEYUKI, K

TANIMORI, T

BEIER, EW

FELDSCHER, LR

FRANK, ED

FRATI, W

KIM, SB

MANN, AK

NEWCOMER, FM

VANBERG, R

ZHANG, W

机构：

[1] KEK NAT LAB HIGH ENERGY PHYS,NATL LAB HIGH ENERGY PHYS,TSUKUBA,IBARAKI 305,JAPAN

[2] TOKAI UNIV,SHIBUYA,TOKYO 151,JAPAN

[3] KOBE UNIV,DEPT PHYS,KOBE,HYOGO 657,JAPAN

[4] NIIGATA UNIV,NIIGATA 95021,JAPAN

[5] OSAKA UNIV,DEPT PHYS,TOYONAKA,OSAKA 560,JAPAN

[6] TOKYO INST TECHNOL,DEPT PHYS,MEGURO KU,TOKYO 152,JAPAN

[7] UNIV PENN,DEPT PHYS,PHILADELPHIA,PA 19104

来源：

PHYSICAL REVIEW LETTERS | 1990年 / 65卷 / 11期

关键词：

D O I：

10.1103/PhysRevLett.65.1301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

An analysis of the Mikheyev-Smirnov-Wolfenstein effect using 1040 days of Kamiokande-II data is reported, which provides constraints on neutrino-oscillation parameters. The measured recoil-electron energy spectrum alone leads to the conclusion that the adiabatic region, 7.2×10-4<sin22 <6.3×10-3, 1.3×10-4 (eV)2, is disfavored at the 90% confidence level. © 1990 The American Physical Society.

引用

页码：1301 / 1304

页数：4

共 19 条

[1] RESONANT AMPLIFICATION OF NEUTRINO SPIN ROTATION IN MATTER AND THE SOLAR-NEUTRINO PROBLEM [J].

AKHMEDOV, EK .

PHYSICS LETTERS B, 1988, 213 (01) :64-68

[2] SOLAR MODELS, NEUTRINO EXPERIMENTS, AND HELIOSEISMOLOGY [J].

BAHCALL, JN ;

ULRICH, RK .

REVIEWS OF MODERN PHYSICS, 1988, 60 (02) :297-372

[3] MATTER-ENHANCED NEUTRINO OSCILLATIONS IN THE STANDARD SOLAR MODEL [J].

BAHCALL, JN ;

HAXTON, WC .

PHYSICAL REVIEW D, 1989, 40 (04) :931-941

[4] SOLAR-NEUTRINO EXPERIMENTS [J].

BETHE, HA .

PHYSICAL REVIEW LETTERS, 1989, 63 (08) :837-839

[5]

DAVIS R, 1989, 13TH P INT C NEUTR P, P518

[6]

DAVIS R, 1987, 7TH P WORKSH GRAND U, P237

[7] OBSERVATION OF 8B-SOLAR NEUTRINOS IN THE KAMIOKANDE-II DETECTOR [J].

HIRATA, KS ;

KAJITA, T ;

KIFUNE, K ;

KIHARA, K ;

NAKAHATA, M ;

NAKAMURA, K ;

OHARA, S ;

OYAMA, Y ;

SATO, N ;

TAKITA, M ;

TOTSUKA, Y ;

YAGINUMA, Y ;

MORI, M ;

SUZUKI, A ;

TAKAHASHI, K ;

TANIMORI, T ;

YAMADA, M ;

KOSHIBA, M ;

SUDA, T ;

MIYANO, K ;

MIYATA, H ;

TAKEI, H ;

KANEYUKI, K ;

NAGASHIMA, Y ;

SUZUKI, Y ;

BEIER, EW ;

FELDSCHER, LR ;

FRANK, ED ;

FRATI, W ;

KIM, SB ;

MANN, AK ;

NEWCOMER, FM ;

VANBERG, R ;

ZHANG, W .

PHYSICAL REVIEW LETTERS, 1989, 63 (01) :16-19

[8] RESULTS FROM 1000 DAYS OF REAL-TIME, DIRECTIONAL SOLAR-NEUTRINO DATA [J].