On fast neutrino flavor conversion modes in the nonlinear regime

被引:68
作者
Abbar, Sajad [1 ]
Volpe, Maria Cristina [1 ]
机构
[1] Univ Paris 07, CNRS UMR 7164, APC, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France
关键词
Neutrino oscillations; Core-collapse supernova; Binary neutron star mergers; INSTABILITIES;
D O I
10.1016/j.physletb.2019.02.002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A dense neutrino medium could experience self-induced flavor conversions on relatively small scales in the presence of the so-called fast flavor conversion modes. Owing to the fact that fast conversion scales could be much smaller than the ones of the traditional collective neutrino oscillations, it has been speculated that fast modes could lead to some sort of flavor decoherence/equilibrium. We study the evolution of fast modes in the nonlinear regime and we show that not only fast modes are not guaranteed to lead to flavor equilibrium, but also they could lead to some sort of collective neutrino oscillations but on scales determined by neutrino number density. For the v(e) dominated case, we observe large amplitude collective oscillations, whereas a sort of flavor stabilization is reached for the (v) over bar (e) dominated case. (C) 2019 The Authors. Published by Elsevier B.V.
引用
收藏
页码:545 / 550
页数:6
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