SOLAR AND SUPERNOVA NEUTRINO PHYSICS WITH SUDBURY-NEUTRINO-OBSERVATORY

被引：20

作者：

BALANTEKIN, AB

LORETI, F

机构：

[1] Physics Department, University of Wisconsin, Madison

来源：

PHYSICAL REVIEW D | 1992年 / 45卷 / 04期

关键词：

D O I：

10.1103/PhysRevD.45.1059

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The salient features of solar and supernova neutrino physics at the Sudbury Neutrino Observatory are examined. The possibility of detecting a solar-antineutrino flux, predicted as a result of resonant spin-flavor conversion, is emphasized. The antineutrino flux at Sudbury due to the commercial power reactors is calculated. Simplified, analytical expressions for the expected galactic supernova count rates are given.

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页码：1059 / 1065

页数：7

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