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The effects originated in dispersion with time on spreading of wave packets for the time-integrated two-flavor neutrino oscillation probabilities in vacuum are studied in the context of a field theory treatment. The neutrino flavor states…

高能物理 - 唯象学 · 物理学 2014-01-10 Y. F. Perez , C. J. Quimbay

Slow flavor evolution (defined as driven by neutrino masses and not necessarily ``slow'') is receiving fresh attention in the context of compact astrophysical environments. In Part~I of this series, we have studied the slow-mode dispersion…

高能物理 - 唯象学 · 物理学 2025-06-03 Damiano F. G. Fiorillo , Georg G. Raffelt

Neutrino oscillations in the early Universe prior to the epoch of primordial nucleosynthesis is studied by implementing real time non-equilibrium field theory methods. We focus on two flavors of Dirac neutrinos, however, the formulation is…

高能物理 - 唯象学 · 物理学 2009-11-11 C. M. Ho , D. Boyanovsky , H. J. de Vega

We study the oscillations and conversions of relativistic neutrinos propagating in matter of variable density using the wave packet formalism. We show how the oscillation and coherence lengths are modified in comparison with the case of…

高能物理 - 唯象学 · 物理学 2011-07-19 J. T. Peltoniemi , V. Sipilainen

Recently the issue of EPR-like correlations in the mutual probability of detecting neutrino together with accompanying charged lepton has received a new impetus. In this paper we describe this effect using the propagators of the particles…

高能物理 - 唯象学 · 物理学 2009-10-30 Yuri Shtanov

In dense neutrino backgrounds present in supernovae and in the early Universe, neutrino oscillations may exhibit complex collective phenomena, such as synchronized oscillations, bipolar oscillations and spectral splits and swaps. In this…

高能物理 - 唯象学 · 物理学 2017-03-02 Evgeny Akhmedov , Joachim Kopp , Manfred Lindner

Neutrino propagation in the Galactic and extragalactic magnetic fields is considered. We extend an approach developed in \cite{Popov:2019nkr} to describe neutrino flavour and spin oscillations using wave packets. The evolution equations for…

高能物理 - 唯象学 · 物理学 2025-05-14 Artem Popov , Alexander Studenikin

We present a pedagogical discussion on the time evolution of a Gaussian neutrino wave packet in free space. A common treatment is to keep momentum terms up to the quadratic order in the expansion of the energy-momentum relation so that the…

高能物理 - 唯象学 · 物理学 2015-03-27 Cheng-Hsien Li , Yong-Zhong Qian

In neutrino-dense astrophysical environments, these particles exchange flavor through a coherent weak field, forming a collisionless neutrino plasma with collective flavor dynamics. Instabilities, which grow and affect the environment, may…

高能物理 - 唯象学 · 物理学 2026-03-31 Damiano F. G. Fiorillo , Georg G. Raffelt

The most general case of self-induced neutrino flavor evolution is described by a set of kinetic equations for a dense neutrino gas evolving both in space and time. Solutions of these equations have been typically worked out assuming that…

高能物理 - 唯象学 · 物理学 2015-06-19 Gianpiero Mangano , Alessandro Mirizzi , Ninetta Saviano

In Phys. Rev. D77 (2008) 105001, we have studied decoherence models for flavour oscillations in four-dimensional stochastically fluctuating space times and discussed briefly the sensitivity of current terrestrial and astrophysical neutrino…

高能物理 - 唯象学 · 物理学 2013-05-29 J. Alexandre , K. Farakos , N. E. Mavromatos , P. Pasipoularides

An electromagnetic wave-packet propagating in a linear, homogeneous, and isotropic medium changes shape while its envelope travels with different velocities at different points in spacetime. In general, a wave-packet can be described as a…

光学 · 物理学 2020-08-26 Masud Mansuripur

The time evolution of anharmonic molecular wave packets is investigated under the influence of the environment consisting of harmonic oscillators. These oscillators represent photon or phonon modes and assumed to be in thermal equilibrium.…

量子物理 · 物理学 2015-06-26 Peter Foldi , Mihaly G. Benedict , Attila Czirjak , Balazs Molnar

At high densities in compact astrophysical sources, the coherent forward scattering of neutrinos onto each other is responsible for making the flavor evolution non-linear. Under the assumption of spherical symmetry, we present the first…

高能天体物理现象 · 物理学 2023-04-05 Shashank Shalgar , Irene Tamborra

We study decoherence effects in neutrino flavour oscillations in curved spacetime with particular emphasis on the lensing in a Schwarzschild geometry. Assuming Gaussian wave packets for neutrinos, we argue that the decoherence length…

高能物理 - 唯象学 · 物理学 2021-11-12 Himanshu Swami , Kinjalk Lochan , Ketan M. Patel

We study the time evolution of the distribution functions for hot and or degenerate gases of two flavors of Dirac neutrinos as a result of flavor mixing and dephasing. This is achieved by obtaining the time evolution of the flavor density…

高能物理 - 唯象学 · 物理学 2009-11-10 D. Boyanovsky , C. M. Ho

The flavor evolution of neutrinos in dense astrophysical sources, such as core-collapse supernovae or compact binary mergers, is non-linear due to the coherent forward scattering of neutrinos among themselves. Recent work in this context…

高能天体物理现象 · 物理学 2024-02-23 Marie Cornelius , Shashank Shalgar , Irene Tamborra

There is renewed attention to whether we can observe the decoherence effect in neutrino oscillation due to the separation of wave packets with different masses in near-future experiments. As a contribution to this endeavor, we extend the…

高能物理 - 唯象学 · 物理学 2023-10-18 Haruhi Mitani , Kin-ya Oda

One of the most common expectations of a quantum theory of gravity is that space-time is uncertain or fluctuating at microscopic scales, making it a stochastic medium for particle propagation. Particles traversing this space-time may…

高能物理 - 唯象学 · 物理学 2022-01-19 Thomas Stuttard

Using a density matrix description in space we study the evolution of wavepackets in a fluctuating space-time background. We assume that space-time fluctuations manifest as classical fluctuations of the metric. From the non-relativistic…

广义相对论与量子宇宙学 · 物理学 2010-04-30 E. Göklü , C. Lämmerzahl , A. Camacho , A. Macias
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