RESULTS FROM SAGE-II

被引：40

作者：

ABDURASHITOV, JN

FAIZOV, EL

GAVRIN, VN

GUSEV, AO

KALIKHOV, AV

KNODEL, TV

KNYSHENKO, II

KORNOUKHOV, VN

MIRMOV, IN

PSHUKOV, AM

SHALAGIN, AM

SHIKHIN, AA

TIMOFEYEV, PV

VERETEKIN, EP

VERMUL, VM

ZATSEPIN, GT

BOWLES, TJ

NICO, JS

TEASDALE, WA

WARK, DL

WILKERSON, JF

CLEVELAND, BT

DAVIS, R

DAILY, T

LANDE, K

LEE, CK

WILDENHAIN, PW

ELLIOTT, SR

CHERRY, ML

机构：

[1] RUSSIAN ACAD SCI,INST NUCL RES,MOSCOW 117312,RUSSIA

[2] LOS ALAMOS NATL LAB,LOS ALAMOS,NM 87545

[3] UNIV PENN,PHILADELPHIA,PA 19104

[4] LAWRENCE LIVERMORE NATL LAB,LIVERMORE,CA 94550

[5] LOUISIANA STATE UNIV,BATON ROUGE,LA 70803

来源：

NUCLEAR PHYSICS B | 1995年

基金：

美国国家科学基金会; 俄罗斯基础研究基金会;

关键词：

D O I：

10.1016/0920-5632(94)00734-D

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：

The Russian-American Gallium solar neutrino Experiment (SAGE) began the second phase of operation (SAGE II) in September of 1992. Monthly measurements of the integral flux of solar neutrinos have been made with 55 tonnes of gallium. The K-peak results of the first five runs of SAGE II give a capture rate of 76+21/-18(stat)+5/-7(syst)SNU. Combined with the SAGE I result, the capture rate is 74+13/-12(stat)+5/-7(syst)SNU. This represents only 56%-60% of the capture rate predicted by different Standard Solar Models.

引用

页码：60 / 67

页数：8

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