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
AKHMEDOV, EK
[J]. PHYSICS LETTERS B, 1988, 213 (01) : 64 - 68
[2] SOLAR MODELS, NEUTRINO EXPERIMENTS, AND HELIOSEISMOLOGY
BAHCALL, JN
ULRICH, RK
[J]. REVIEWS OF MODERN PHYSICS, 1988, 60 (02) : 297 - 372
[3] MATTER-ENHANCED NEUTRINO OSCILLATIONS IN THE STANDARD SOLAR MODEL
BAHCALL, JN
HAXTON, WC
[J]. PHYSICAL REVIEW D, 1989, 40 (04): : 931 - 941
[4] SOLAR-NEUTRINO EXPERIMENTS
BETHE, HA
[J]. 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
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
[J]. PHYSICAL REVIEW LETTERS, 1989, 63 (01) : 16 - 19
[8] RESULTS FROM 1000 DAYS OF REAL-TIME, DIRECTIONAL SOLAR-NEUTRINO DATA
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
[J]. PHYSICAL REVIEW LETTERS, 1990, 65 (11) : 1297 - 1300
[9] HIRATA KS, 1989, 14TH P INT S LEPT PH
[10] SOLAR NEUTRINO OBSERVATIONS AND NEUTRINO OSCILLATIONS
KUO, TK
PANTALEONE, J
[J]. PHYSICAL REVIEW D, 1990, 41 (12): : 3842 - 3845

← 1 2 →