Running neutrino mass parameters in see-saw scenarios

被引:304
作者
Antusch, S [1 ]
Kersten, J
Linder, M
Ratz, M
Schmidt, MA
机构
[1] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[2] Deutsch Elektronen Synchotron DESY, D-22603 Hamburg, Germany
[3] Tech Univ Munich, Dept Phys T30, D-85748 Garching, Germany
[4] Univ Bonn, Inst Phys, D-53115 Bonn, Germany
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2005年 / 03期
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
renormalization group; beyond standard model; supersymmetric standard model; neutrino physics;
D O I
10.1088/1126-6708/2005/03/024
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We synthematically analyze quantum corrections in see-saw scenarios, including effects from above as well as below the see-saw scales. We derive approximate renormalization group equations for neutrino masses, lepton mixings and CP phases, yielding an analytic understanding and a simple estimate of the size of the effects. Even for hierarchical masses, they often exceed the precision of future experiments. Furthermore, we provide a software package allowing for a convenient numerical renormalization group analysis, with heavy singlets being integrated out successively at their mass thresholds. We also discuss applications to model building and related topics.
引用
收藏
页码:553 / 603
页数:51
相关论文
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