Identifying the neutrino mass spectrum from a supernova neutrino burst

被引：487

作者：

Dighe, AS ^{[1
]}

Smirnov, AY

机构：

[1] CERN, Div Theory, CH-1211 Geneva 23, Switzerland

[2] Abdus Salam Int Ctr Theoret Phys, I-34100 Trieste, Italy

[3] Russian Acad Sci, Inst Nucl Res, Moscow, Russia

来源：

PHYSICAL REVIEW D | 2000年 / 62卷 / 03期

关键词：

D O I：

10.1103/PhysRevD.62.033007

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the role that the future detection of the neutrino burst from a galactic supernova can play in the reconstruction of the neutrino mass spectrum. We consider all possible 3v mass and flavor spectra which describe the solar and atmospheric neutrino data. For each of these spectra we find the observable effects of the supernova neutrino conversions both in the matter of the star and the Earth. We show that studies of the electron neutrino and antineutrino spectra as well as observations of the neutral current effects from supernova will allow us (i) to identify the solar neutrino solution, (ii) to determine the type of mass hierarchy (normal or inverted) and (iii) to probe the mixing \ U-e3\(2) to values as low as 10(-4)-10(-3).

引用

页数：24

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