MONTE-CARLO EXPLORATION OF MIKHEYEV-SMIRNOV-WOLFENSTEIN SOLUTIONS TO THE SOLAR NEUTRINO PROBLEM

被引：64

作者：

SHI, X

SCHRAMM, DN

BAHCALL, JN

机构：

[1] NASA,FERMILAB ASTROPHYS CTR,FERMI NATL ACCELERATOR LAB,BATAVIA,IL 60510

[2] INST ADV STUDY,PRINCETON,NJ 08540

来源：

PHYSICAL REVIEW LETTERS | 1992年 / 69卷 / 05期

关键词：

D O I：

10.1103/PhysRevLett.69.717

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We explore the impact of astrophysical uncertainties on the Mikheyev-Smirnov-Wolfenstein (MSW) solution by calculating the allowed MSW solutions for 1000 different solar models with a Monte Carlo selection of solar model input parameters, assuming a full three-family MSW mixing. Applications are made to the chlorine, gallium, Kamiokande, and Borexino experiments. The initial GALLEX result limits the mixing parameters to the upper diagonal and the vertical regions of the MSW triangle. We also calculate the expected event rates in the Borexino experiment assuming the MSW solutions implied by GALLEX.

引用

页码：717 / 720

页数：4

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