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相关论文: Chameleon-neutrino conformal coupling and MSW-medi…

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Flavor transitions of Neutrinos with a nonstandard interaction are studied. A scalar field is conformally coupled to matter and neutrinos. This interaction alters the neutrino effective mass and its wavefunction leading to a damping factor,…

高能物理 - 唯象学 · 物理学 2021-05-25 H. Mohseni Sadjadi , H. Yazdani Ahmadabadi

In screening models with scalar-matter conformal coupling, we study the flavor transition of neutrinos. We employ an analytical method for studying the oscillation phase in a spherically symmetric spacetime filled by a scalar field. Since…

高能物理 - 唯象学 · 物理学 2022-06-17 H. Yazdani Ahmadabadi , H. Mohseni Sadjadi

Matter-induced neutrino flavor mixing (the Mikheyev-Smirnov-Wolfenstein, or MSW, effect) is a central prediction of the neutrino mixing framework, but it has not been conclusively observed. Direct observation of the energy-dependent MSW…

高能物理 - 唯象学 · 物理学 2026-02-02 Obada Nairat , John F. Beacom , Kevin J. Kelly , Shirley Weishi Li

We study the effects of a scalar field, coupled only to neutrinos, on oscillations among weak interaction current eigenstates. The effect of a real scalar field appears as effective masses for the neutrino mass eigenstates, the same for…

高能物理 - 唯象学 · 物理学 2008-11-26 G. J. Stephenson , T. Goldman , B. H. J. McKellar

A proposal for the neutrino mass, based on neutrino-scalar field interaction, is introduced. The scalar field is also non-minimally coupled to the Ricci scalar and hence relates the neutrino mass to the matter density. In a dense region,…

高能物理 - 唯象学 · 物理学 2018-04-17 H. Mohseni Sadjadi , A. P. Khosravi Karchi

We examine the effects of a scalar field, coupled only to neutrinos, on oscillations among weak interaction current eigenstates. The existence of a real scalar field is manifested as effective masses for the neutrino mass eigenstates, the…

高能物理 - 唯象学 · 物理学 2007-05-23 T. Goldman , B. H. J. McKellar , G. J. Stephenson

We recently studied neutrinos flavor oscillations in vacuum within conformal coupling models. In this paper, we extend that analysis by investigating neutrino flavor oscillations inside matter within a general conformal coupling scenario.…

高能物理 - 唯象学 · 物理学 2023-05-15 Fayçal Hammad , Parvaneh Sadeghi , Nicolas Fleury

We consider flavor changing effective neutrino interactions in the context of massive neutrinos in the issue of atmospheric neutrinos. Assuming as usual that this is an indication of the oscillation of muon neutrinos into tau neutrinos we…

高能物理 - 唯象学 · 物理学 2007-05-23 J. C. Montero , V. Pleitez

The MSW (Mikheyev-Smirnov-Wolfenstein) effect is the adiabatic or partially adiabatic neutrino flavor conversion in medium with varying density. The main notions related to the effect, its dynamics and physical picture are reviewed. The…

高能物理 - 唯象学 · 物理学 2009-11-10 A. Yu. Smirnov

We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, delta-correlated matter density. The fluctuations will produce a distribution of neutrino survival probabilities. We find the mean and…

天体物理学 · 物理学 2008-11-26 A. B. Balantekin , J. M. Fetter , F. N. Loreti

We present a theory of neutrino oscillations in a dense medium which goes beyond the effective matter potential used in the description of the MSW effect. We show how the purity of the neutrino state is degraded by neutrino interactions…

高能物理 - 唯象学 · 物理学 2021-07-20 Antonio Capolupo , Salvatore Marco Giampaolo , Aniello Quaranta

Regarding the proximity of dark energy scale and neutrino mass, one can get new insight into the probe signatures of vector field dark energy component on neutrino flavor conversion. A vector field is assumed to be conformally coupled to…

高能物理 - 唯象学 · 物理学 2024-11-19 H. Yazdani Ahmadabadi , H. Mohseni Sadjadi

In this paper, we study the spin transitions of neutrinos caused by the interaction with a gravitational field. We consider a model with a scalar field (describing screening effects) conformally coupled to matter and neutrinos. The presence…

广义相对论与量子宇宙学 · 物理学 2021-07-12 Leonardo Mastrototaro , Gaetano Lambiase

We consider a class of models involving interactions between ultra-light scalar dark matter and Standard Model neutrinos. Such couplings modify the neutrino mass splittings and mixing angles to include additional components that vary in…

高能物理 - 唯象学 · 物理学 2016-12-07 Asher Berlin

The MSW (Mikheyev-Smirnov-Wolfenstein) effect is the effect of transformation of one neutrino species (flavor) into another one in a medium with varying density. Three basic elements of the effect include: the refraction of neutrinos in…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Yu. Smirnov

Effects of the dense matter can induce the neutrino decay even if neutrinos are stable in vacuum. This is due to coherent interactions with matter which lead to energy level-splitting between the neutrino and antineutrino states and thereby…

高能物理 - 唯象学 · 物理学 2007-05-23 Zurab G. Berezhiani , Anna Rossi

A super-light sterile neutrino was proposed to explain the absence of the expected upturn of the survival probability of low energy solar boron neutrinos. This is because this super-light sterile neutrino can oscillate efficiently with…

高能物理 - 唯象学 · 物理学 2015-06-19 Wei Liao , Yuchen Luo , Xiao-Hong Wu

Sterile neutrinos at the eV scale have long been studied in the context of anomalies in short baseline neutrino experiments. Their cosmology can be made compatible with our understanding of the early Universe provided the sterile neutrino…

高能物理 - 唯象学 · 物理学 2017-07-26 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

We study some implications on standard matter oscillations of solar neutrinos induced by a background of extremely low energy thermal neutrinos trapped inside the Sun by means of coherent refractive interactions. Possible experimental tests…

高能物理 - 唯象学 · 物理学 2011-09-12 S. Esposito

We point out that the recent data from the Sudbury Neutrino Observatory, together with other relevant measurements from solar and reactor neutrino experiments, convincingly show that the flavor transitions of solar neutrinos are affected by…

高能物理 - 唯象学 · 物理学 2009-10-07 G. L. Fogli , E. Lisi , A. Marrone , A Palazzo
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