Slow and fast collective neutrino oscillations: Invariants and reciprocity
arXiv:2301.09650 · doi:10.1103/PhysRevD.107.043024
Abstract
The flavor evolution of a neutrino gas can show ''slow'' or ''fast'' collective motion. In terms of the usual Bloch vectors to describe the mean-field density matrices of a homogeneous neutrino gas, the slow two-flavor equations of motion (EOMs) are , where , , is a unit vector in the mass direction in flavor space, and . For an axisymmetric angle distribution, the fast EOMs are , where is the Bloch vector for lepton number, is the velocity along the symmetry axis, , and . We discuss similarities and differences between these generic cases. Both systems can have pendulum-like instabilities (soliton solutions), both have similar Gaudin invariants, and both are integrable in the classical and quantum case. Describing fast oscillations in a frame comoving with (which itself may execute pendulum-like motions) leads to transformed EOMs that are equivalent to an abstract slow system. These conclusions carry over to three flavors.
16 pages; post-publication corrected treatment of Lax vectors and Gaudin invariants, especially for three-flavor case. Matching the corrections in the Erratum accepted on PRD
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