A SOLUTION OF THE SOLAR-NEUTRINO PROBLEM

被引：193

作者：

BAHCALL, JN ^{[1
]}

BETHE, HA ^{[1
]}

机构：

[1] CORNELL UNIV,NEWMAN LAB NUCL STUDIES,ITHACA,NY 14853

来源：

PHYSICAL REVIEW LETTERS | 1990年 / 65卷 / 18期

关键词：

D O I：

10.1103/PhysRevLett.65.2233

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Comparison of the results from the Kamiokande neutrino-electron scattering experiment with those from the chlorine experiment and with solar models shows that the explanation of the solar-neutrino problem probably requires physics beyond the standard electroweak model with zero neutrino masses. The experimental results, including the shape of the electron-recoil energy spectrum measured by Kamiokande, are in excellent agreement with a nonadiabatic solution of the Mikheyev-Smirnov-Wulfenstein effect, yielding a neutrino mass difference of m2=1×10-8 sin-2V eV2. © 1990 The American Physical Society.

引用

页码：2233 / 2235

页数：3

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