Solar neutrinos and neutrino physics

被引：73

作者：

Maltoni, Michele ^{[1
]}

Smirnov, Alexei Yu. ^{[2
,3
]}

机构：

[1] Univ Autonoma Madrid, CSIC, Inst Fis Teor UAM, Calle Nicolas Cabrera 13-15, E-28049 Madrid, Spain

[2] Max Planck Inst Nucl Phys, Saupfercheckweg 1, D-69117 Heidelberg, Germany

[3] Abdus Salaam Int Ctr Theoret Phys, Str Costiera 11, I-34014 Trieste, Italy

来源：

EUROPEAN PHYSICAL JOURNAL A | 2016年 / 52卷 / 04期

关键词：

MAGNETIC-MOMENT; RESONANT AMPLIFICATION; OSCILLATIONS; MATTER; CONSERVATION; SEARCH; BOUNDS;

D O I：

10.1140/epja/i2016-16087-0

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Solar neutrino studies triggered and largely motivated the major developments in neutrino physics in the last 50 years. The theory of neutrino propagation in different media with matter and fields has been elaborated. It includes oscillations in vacuum and matter, resonance flavor conversion and resonance oscillations, spin and spin-flavor precession, etc. LMA MSW has been established as the true solution of the solar neutrino problem. Parameters theta(12) and Delta m(21)(2) have been measured; theta(13) extracted from the solar data is in agreement with results from reactor experiments. Solar neutrino studies provide a sensitive way to test theory of neutrino oscillations and conversion. Characterized by long baseline, huge fluxes and low energies they are a powerful set-up to search for new physics beyond the standard 3v paradigm: new neutrino states, sterile neutrinos, non-standard neutrino interactions, effects of violation of fundamental symmetries, new dynamics of neutrino propagation, probes of space and time. These searches allow us to get stringent, and in some cases unique bounds on new physics. We summarize the results on physics of propagation, neutrino properties and physics beyond the standard model obtained from studies of solar neutrinos.

引用

页数：16

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