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相关论文: A Theory of Neutrino Oscillations and Late Time Ac…

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If dark energy (DE) couples to neutrinos, then there may be apparent violations of Lorentz/CPT invariance in neutrino oscillations. The DE-induced Lorentz/CPT violation takes a specific form that introduces neutrino oscillations that are…

高能物理 - 唯象学 · 物理学 2010-04-29 Shin'ichiro Ando , Marc Kamionkowski , Irina Mocioiu

If dark energy (DE) is a dynamical field rather than a cosmological constant, an interaction between DE and the neutrino sector could exist, modifying the neutrino oscillation phenomenology and causing CP and apparent Lorentz violating…

高能物理 - 唯象学 · 物理学 2018-03-14 Niki Klop , Shin'ichiro Ando

As the increasing of neutrino energy or matter density, the neutrino oscillation in matter may undergo "vacuum-dominated", "resonance" and "matter-dominated" three different stages successively. Neutrinos endure very different matter…

高能物理 - 唯象学 · 物理学 2020-02-26 Shu Luo

In this review, I discuss briefly how the presence of a cosmological constant in the Universe may imply a decoherent evolution of quantum matter in it, and as a consequence a fundamental irreversibility of time unrelated in principle to CP…

广义相对论与量子宇宙学 · 物理学 2007-05-23 N. E. Mavromatos

We present analytical solutions to the nonlinear equations describing the behavior of a gas of neutrinos with two flavors. Self-maintained coherent flavor oscillations are shown to occur when the gas density exceeds a critical value…

高能物理 - 唯象学 · 物理学 2009-09-25 Alan Kostelecky , Stuart Samuel

Neutrino oscillations is a phenomenon which is characterized by a finite oscillation time (length). For such phenomena time-energy uncertainty relation is valid. This means that energy uncertainty is needed for oscillations to occur. We…

高能物理 - 唯象学 · 物理学 2007-05-23 S. M. Bilenky

Phenomenology of neutrino oscillations in vacuum and in cosmological plasma is considered. Neutrino oscillations in vacuum are usually described in plane wave approximation. In this formalism there is an ambiguity if one should assume…

高能物理 - 唯象学 · 物理学 2007-05-23 A. D. Dolgov

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. We consider…

高能物理 - 唯象学 · 物理学 2016-05-23 Evgeny Akhmedov , Alessandro Mirizzi

Neutrino oscillations in a hot and dense astrophysical environment such as a core-collapse supernova pose a challenging, seven-dimensional flavor transport problem. To make the problem even more difficult (and interesting), neutrinos can…

高能物理 - 唯象学 · 物理学 2015-09-11 Huaiyu Duan

The emerging structure of the neutrino mass matrix, when combined with the primordial element abundances, places the most stringent constraint on the flavor asymmetries in the cosmological neutrino background and therefore its energy…

高能物理 - 唯象学 · 物理学 2009-11-10 Kevork Abazajian

Existing experimental data for neutrino oscillations are consistent with Lorentz-violating massless neutrinos. This talk summarizes some aspects of neutrino oscillations from the perspective of Lorentz and CPT violation in effective quantum…

高能物理 - 唯象学 · 物理学 2007-05-23 Alan Kostelecky

In this paper we study the dynamical CPT violation in the neutrino sector induced by the dark energy of the Universe. Specifically we consider a dark energy model where the dark energy scalar derivatively interacts with the right-handed…

高能物理 - 唯象学 · 物理学 2008-11-26 Pei-Hong Gu , Xiao-Jun Bi , Xinmin Zhang

A number of derivations of the standard neutrino oscillation formula are known, each one providing its own unique insights. Common to all treatments is the assumption that neutrinos propagate freely between source and detector, as indeed…

高能物理 - 唯象学 · 物理学 2019-10-08 Lucas Johns

Dense neutrino gases exhibit collective oscillations where "self-maintained coherence" is a characteristic feature, i.e., neutrinos of different energies oscillate with the same frequency. In a non-isotropic gas, however, the flux term of…

高能物理 - 唯象学 · 物理学 2008-11-26 G. G. Raffelt , G. Sigl

We show that when the neutrino minimal standard model ($\nu MSM$) with a light sterile neutrino has a long range interaction between the neutrino vacuum charge density and a dark U(1) gauge potential, late time acceleration is dynamically…

高能物理 - 唯象学 · 物理学 2013-06-14 Stephon H. S. Alexander

The neutrino propagating in curved spacetimes, e.g. around black holes, in early curved universe, violates Lorentz and then CPT symmetry, at least in the local coordinate. This occurs due to coupling of spin of the neutrino to background…

广义相对论与量子宇宙学 · 物理学 2016-11-15 Banibrata Mukhopadhyay

Space-time localization diagrams ``unlock" subtle aspects of $\nu$ oscillations such as coherence and entanglement. Observability of propagation decoherence in oscillating neutrino state is discussed. The sizes of WPs of reactor and source…

高能物理 - 唯象学 · 物理学 2022-12-21 Alexei Y Smirnov

We propose that gravitational interactions of cosmic neutrinos with the statistically homogeneous and isotropic fluctuations of space-time leads to decoherence. This working hypothesis, which we describe by means of a Lindblad operator, is…

宇宙学与河外天体物理 · 物理学 2019-08-06 Daniel Boriero , Dominik J. Schwarz , Hermano Velten

Lorentz invariance is a well known fundamental concept of special relativity but its violation is predicted by some variations of quantum gravity, string theory, and some alternatives to general relativity. We study neutrino oscillation at…

高能物理 - 唯象学 · 物理学 2016-12-30 S. A. Alavi , M. Dehghani Madise

We present cosmological perturbation theory in neutrinos probe interacting dark-energy models, and calculate cosmic microwave background anisotropies and matter power spectrum. In these models, the evolution of the mass of neutrinos is…

天体物理学 · 物理学 2009-06-23 Kiyotomo Ichiki , Yong-Yeon Keum
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