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相关论文: Gravitational coupling of neutrinos in a medium

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When neutrinos travel through a normal matter medium, the electron neutrinos couple differently to gravity compared to the other neutrinos, due to the presence of electrons in the medium and the absence of the other charged leptons. The…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Jose F. Nieves , Palash B. Pal

We calculate the leading order matter-induced corrections to the gravitational interactions of charged leptons and their antiparticles in a medium that contains electrons but not the other charged leptons, such as normal matter. The…

高能物理 - 唯象学 · 物理学 2009-11-07 Indrajit Mitra , Jose F. Nieves , Palash B. Pal

When neutrinos propagate in a background, their gravitational couplings are modified by their weak interactions with the particles in the background. In a medium that contains electrons but no muons or taons, the matter-induced…

高能物理 - 唯象学 · 物理学 2010-12-03 H. Athar , Jose F. Nieves

When neutrinos travel through a normal matter medium, the electron neutrinos couple differently to gravity compared to the other neutrinos, due to the presence of electrons in the medium and the absence of the other charged leptons. We…

高能物理 - 唯象学 · 物理学 2009-10-31 Jose F. Nieves , Palash B. Pal

In this work we propose an extended formulation for the interaction between neutrinos and gravitational fields. It is based on the parametrized post-Newtonian aproach, and includes a violation of the universality of the gravitational…

高能物理 - 唯象学 · 物理学 2009-12-30 H. Casini , J. C. D'Olivo , R. Montemayor , L. F. Urrutia

We look at the possibility that appreciable neutrino masses and flavor mixing occur only within material media, driven by an interaction between leptons and a very light scalar particle. Limits are placed on the scalar particle mass and…

高能物理 - 唯象学 · 物理学 2009-10-31 R. F. Sawyer

Neutrinos propagating in media (matter and electromagnetic fields) undergo flavor and helicity oscillations, where helicity transitions are instigated both by electromagnetic fields and matter currents. In addition, it has been shown that…

高能物理 - 唯象学 · 物理学 2015-06-18 A. Kartavtsev , G. Raffelt , H. Vogel

We study spin and flavor oscillations of astrophysical neutrinos under the influence of external fields in curved spacetime. First, we consider spin oscillations in case of neutrinos gravitationally scattered off a rotating supermassive…

高能物理 - 唯象学 · 物理学 2023-06-01 Maxim Dvornikov

Neutrinos do oscillate, which up to our best knowledge implies that they are massive particles. As such, neutrinos should interact with gravitational fields. As their masses are tiny, the gravitational fields must be extremely strong. In…

高能物理 - 唯象学 · 物理学 2015-06-03 Marek Góźdź , Marek Rogatko

We present the results on non-perturbative quantum gravity effects related to extra dimensions which can be comparable, in some cases, with the SM contributions, e.g. in lepton-lepton or lepton-nucleon scattering. The case of cosmic…

高能物理 - 唯象学 · 物理学 2009-11-10 A. V. Kisselev , V. A. Petrov

Neutrino flavour oscillations in a nonuniformly moving matter are considered. The neutrino oscillation resonance condition in presence of matter, in the most general case when matter is moving with acceleration, is derived for the first…

高能物理 - 唯象学 · 物理学 2013-12-30 Alexander Studenikin , Ilya Tokarev

Do neutrinos have nonzero masses? If they do, then these masses are very tiny, and can be sought only in very sensitive experiments. The most sensitive of these search for neutrino oscillation, a quantum interference effect which requires…

高能物理 - 唯象学 · 物理学 2017-08-23 Boris Kayser

We study the modification of the detected flavor content of ultra high-energy astrophysical neutrinos in the presence of non-standard interactions of neutrinos with the Earth matter. Unlike the case of new physics affecting the propagation…

高能物理 - 唯象学 · 物理学 2017-02-28 M. C. Gonzalez-Garcia , Michele Maltoni , Ivan Martinez-Soler , Ningqiang Song

The detection and the research of the neutrinos background of Universe are the attractive problems. This problems do not seem the unpromising one in the case of the high neutrinos density of Universe. It is offered to use the low energy…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Valery Koryukin

We consider nonstandard interactions of neutrinos with electrons arising from a new light spin-1 particle with mass of tens of GeV or lower and couplings to the neutrinos and electron. This boson is not necessarily a gauge boson and is…

高能物理 - 唯象学 · 物理学 2013-11-21 Cheng-Wei Chiang , Gaber Faisel , Yi-Fan Lin , Jusak Tandean

Thanks to compelling evidence that neutrinos can change flavor, we now know that they have nonzero masses, and that leptons mix. In these lectures, we explain the physics of neutrino flavor change, both in vacuum and in matter. Then, we…

高能物理 - 唯象学 · 物理学 2008-11-26 Boris Kayser

If a fermion is travelling through a medium, it can have matter-induced magnetic and electric dipole moments. These contributions conserve chirality, and can be non-vanishing even for a Majorana neutrino. Several implications for neutrino…

高能物理 - 唯象学 · 物理学 2007-05-23 Palash B Pal

This letter proposes an alternative quantum mechanical picture for the observed phenomena of neutrino oscillations. It is assumed in the following that neutrinos interact via diabatic (or localised) interactions with a new particle field,…

高能物理 - 唯象学 · 物理学 2020-12-18 M. Bergevin

In the presence of a thermal medium or an external electro-magnetic field, neutrinos can interact with photon, mediated by the corresponding charged leptons (real or virtual). The effect of a medium or an electromagnetic field is two-fold -…

高能物理 - 唯象学 · 物理学 2007-05-23 Kaushik Bhattacharya , Avijit K. Ganguly

The phenomenon of neutrino oscillations has been established as the leading mechanism behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are massive and lepton flavors are mixed. Here we review…

高能物理 - 唯象学 · 物理学 2013-03-21 Tommy Ohlsson
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