Just so neutrino oscillations are back

被引：31

作者：

Glashow, SL ^{[1
]}

Kernan, PJ

Krauss, LM

机构：

[1] Harvard Univ, Lyman Lab Phys, Cambridge, MA 02138 USA

[2] Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA

[3] Case Western Reserve Univ, Dept Astron, Cleveland, OH 44106 USA

来源：

PHYSICS LETTERS B | 1999年 / 445卷 / 3-4期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/S0370-2693(98)01449-X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Recent evidence for oscillations of atmospheric neutrinos at Super-Kamiokande suggest, in the simplest see-saw interpretation, neutrino masses such that "just so" vacuum oscillations can explain the solar neutrino deficit. Super-K solar neutrino data provide preliminary support for this interpretation. We describe how the just-so signal - an energy dependent seasonal variation of the event rate, might be detected within the coming years and provide general arguments constraining the sign of the variation. The expected variation at radiochemical detectors may be below present sensitivity, but a significant modulation in the Be-7 signal could shed light on the physics of the solar core - including a direct measure of the solar core temperature. (C) 1999 Elsevier Science B.V. All rights reserved.

引用

页码：412 / 418

页数：7

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