Collective neutrino oscillations and neutrino wave packets

被引:35
作者
Akhmedov, Evgeny [1 ,4 ]
Kopp, Joachim [2 ,3 ]
Lindner, Manfred [1 ]
机构
[1] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
[2] Johannes Gutenberg Univ Mainz, PRISMA Cluster Excellence, D-55099 Mainz, Germany
[3] Johannes Gutenberg Univ Mainz, Mainz Inst Theoret Phys, D-55099 Mainz, Germany
[4] Natl Res Ctr Kurchatov Inst, Moscow, Russia
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2017年 / 09期
关键词
supernova neutrinos; neutrino theory; SUPERNOVA NEUTRINOS; COHERENCE; MATTER;
D O I
10.1088/1475-7516/2017/09/017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Effects of decoherence by wave packet separation on collective neutrino oscillations in dense neutrino gases are considered. We estimate the length of the wave packets of neutrinos produced in core collapse supernovae and the expected neutrino coherence length, and then proceed to consider the decoherence effects within the density matrix formalism of neutrino flavour transitions. First, we demonstrate that for neutrino oscillations in vacuum the decoherence effects are described by a damping term in the equation of motion of the density matrix of a neutrino as a whole (as contrasted to that of the fixed-momentum components of the neutrino density matrix). Next, we consider neutrino oscillations in ordinary matter and dense neutrino backgrounds, both in the adiabatic and non-adiabatic regimes. In the latter case we study two specific models of adiabaticity violation one with short-term and another with extended non-adiabaticity. It is demonstrated that, while in the adiabatic case a damping term is present in the equation of motion of the neutrino density matrix (just like in the vacuum oscillation case), no such term in general appears in the non-adiabatic regime.
引用
收藏
页数:37
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