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相关论文: Neutrino mixing as a source of dark energy

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We report on the recent result that a contribution to the dark energy can be achieved by the vacuum condensate induced by neutrino mixing phenomenon.

高能物理 - 理论 · 物理学 2008-11-26 M. Blasone , A. Capolupo , S. Capozziello , G. Vitiello

We report on recent results on particle mixing and oscillations in quantum field theory. We discuss the role played in cosmology by the vacuum condensate induced by the neutrino mixing phenomenon. We show that it can contribute to the dark…

高能物理 - 理论 · 物理学 2008-09-02 M. Blasone , A. Capolupo , S. Capozziello , G. Vitiello

We shortly summarize the quantum field theory formalism for the neutrino mixing and report on recent results showing that the vacuum condensate induced by neutrino mixing can be interpreted as a dark energy component of the Universe.

高能物理 - 理论 · 物理学 2008-11-26 M. Blasone , A. Capolupo , S. Capozziello , G. Vitiello

The energy content of the vacuum condensate induced by the neutrino mixing is interpreted as dynamically evolving dark energy.

高能物理 - 理论 · 物理学 2008-11-26 Antonio Capolupo , Salvatore Capozziello , Giuseppe Vitiello

The today estimated value of dark energy can be achieved by the vacuum condensate induced by neutrino mixing phenomenon. Such a tiny value is recovered for a cut-off of the order of Planck scale and it is linked to the sub eV neutrino mass…

高能物理 - 理论 · 物理学 2014-11-18 A. Capolupo , S. Capozziello , G. Vitiello

We show that the non-perturbative vacuum structure associated with neutrino mixing leads to a non-zero contribution to the value of the cosmological constant. Such a contribution comes from the specific nature of the mixing phenomenon. Its…

广义相对论与量子宇宙学 · 物理学 2009-11-10 M. Blasone , A. Capolupo , S. Capozziello , S. Carloni , G. Vitiello

The vacuum condensate due to neutrino and quark mixing behaves as a perfect fluid and, at the present epoch, as a cosmological constant. The very small breaking of the Lorentz invariance constrains today the value of the dark energy.

高能物理 - 理论 · 物理学 2009-07-24 Antonio Capolupo , Giuseppe Vitiello

The mixing of neutrinos and quarks generate a vacuum condensate that, at the present epoch, behaves as a cosmological constant. The value of the dark energy is constrained today by the very small breaking of the Lorentz invariance.

高能物理 - 理论 · 物理学 2014-11-20 Massimo Blasone , Antonio Capolupo , Giuseppe Vitiello

We report on the recent result that the non--perturbative vacuum structure associated with neutrino mixing leads to a non--zero contribution to the value of the cosmological constant. Its value is estimated by using the natural cut--off…

高能物理 - 理论 · 物理学 2016-10-28 Massimo Blasone , Antonio Capolupo , Salvatore Capozziello , Sante Carloni , Giuseppe Vitiello

We report on recent results showing that neutrino mixing may lead to a non-zero contribution to the cosmological constant. This contribution is of a completely different nature with respect to the usual one by a massive spinor field. We…

高能物理 - 理论 · 物理学 2015-06-26 Massimo Blasone , Antonio Capolupo , Salvatore Capozziello , Sante Carloni , Giuseppe Vitiello

Many candidate models for dark energy are based on the existence of a classical scalar field. In the context of Quantum Field Theory (QFT), we briefly discus the condensation of such a field from a light quantum scalar field produced by…

高能物理 - 唯象学 · 物理学 2011-12-19 Houri Ziaeepour

We show that the vacuum condensate due to particle mixing is responsible of a dynamically evolving dark energy. In particular, we show that values of the adiabatic index close to -1 for vacuum condensates of neutrinos and quarks imply, at…

高能物理 - 理论 · 物理学 2009-02-02 A. Capolupo , S. Capozziello , G. Vitiello

It was recently suggested (arxiv:2410.06604) that the small value of the dark energy of the universe could be explained in terms of the scale of neutrino masses through a simple quantum field theoretic mechanism. I clarify that the quantity…

高能物理 - 唯象学 · 物理学 2024-10-17 James M. Cline

Several cosmologically distant astrophysical sources may produce high-energy cosmic neutrinos (E \geq 10^6 GeV) of all flavors above the atmospheric neutrino background. We study the effects of vacuum neutrino mixing in three flavor…

高能物理 - 唯象学 · 物理学 2008-11-26 H. Athar , M. Jezabek , O. Yasuda

Growing neutrino quintessence addresses the "why now" problem of dark energy by assuming that the neutrinos are coupled to the dark energy scalar field. The coupling mediates an attractive force between the neutrinos leading to the…

宇宙学与河外天体物理 · 物理学 2013-03-14 Youness Ayaita , Maik Weber , Christof Wetterich

We propose a new solution to the origin of dark energy. We suggest that it was created dynamically from the condensate of a singlet neutrino at a late epoch of the early Universe through its effective self interaction. This singlet neutrino…

高能物理 - 唯象学 · 物理学 2014-11-20 Jitesh R. Bhatt , Bipin R. Desai , Ernest Ma , G. Rajasekaran , Utpal Sarkar

Astronomical observations indicate an accelerated cosmic expansion, the cause of which is explained by the action of `dark energy'. Here we show that in discrete expanding space-time, only a tiny fraction of the vacuum fluctuations can…

宇宙学与河外天体物理 · 物理学 2012-11-21 Bruno M. Deiss

It is shown that the vacuum condensate induced by many phenomena behaves as a perfect fluid which, under particular conditions, has zero or negative pressure. In particular, the condensates of thermal states, of fields in curved space and…

高能物理 - 理论 · 物理学 2016-10-28 Antonio Capolupo

The quartic-divergent vacuum energy poses an ultraviolet (UV) challenge (the cosmological constant problem) in probing the nature of dark energy. Here we try to evaluate the contribution of the vacuum energy to dark energy with a method of…

高能物理 - 唯象学 · 物理学 2025-12-25 Lian-Bao Jia

Cosmological consequences of a coupling between massive neutrinos and dark energy are investigated. In such models, the neutrino mass is a function of a scalar field, which plays the role of dark energy. The background evolution, as well as…

天体物理学 · 物理学 2010-04-06 A. W. Brookfield , C. van de Bruck , D. F. Mota , D. Tocchini-Valentini
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