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Related papers: MSW-like Enhancements without Matter

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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…

High Energy Physics - Phenomenology · Physics 2007-05-23 T. Goldman , B. H. J. McKellar , G. J. Stephenson

A modified version of the MSW effect is studied within the framework of screening models through conformal couplings of a scalar field within matter. Such a coupling leads to a new, unknown interaction between the scalar field and the…

High Energy Physics - Phenomenology · Physics 2024-08-21 H. Yazdani Ahmadabadi , H. Mohseni Sadjadi

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,…

High Energy Physics - Phenomenology · Physics 2018-04-17 H. Mohseni Sadjadi , A. P. Khosravi Karchi

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. C. Montero , V. Pleitez

A new more rigorous and accurate method for treating neutrino oscillations in the context of the MSW effect in a medium is proposed. This leads to a new type of resonance condition which for small mixing angles puts rather stringent…

High Energy Physics - Phenomenology · Physics 2009-09-25 G. K. Leontaris , J. D. Vergados

We show in detail the general relationship between the Schr\"{o}dinger equation approach to calculating the MSW effect and the quantum field theoretical S-matrix approach. We show the precise form a generic neutrino propagator must have to…

High Energy Physics - Phenomenology · Physics 2009-10-31 Christian Y. Cardall , Daniel J. H. Chung

We point out that the length scale associated with the MSW effect is the radius of the Earth. Therefore to verify matter enhancement of neutrino oscillations, it will be necessary to study neutrinos passing through the Earth. For the…

High Energy Physics - Phenomenology · Physics 2009-10-30 James M. Gelb , Waikwok Kwong , S. P. Rosen

Consequences of a new force mediated by a light scalar particle for neutrino oscillation experiments are considered. Such a force could give rise to neutrino masses and mixings whose matter dependence is much more significant than the MSW…

High Energy Physics - Phenomenology · Physics 2008-11-26 Kathryn M. Zurek

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…

High Energy Physics - Phenomenology · Physics 2009-11-10 A. Yu. Smirnov

Non-standard interactions (NSI) of neutrinos with matter mediated by a scalar field would induce medium-dependent neutrino masses which can modify oscillation probabilities. Generating observable effects requires an ultra-light scalar…

High Energy Physics - Phenomenology · Physics 2020-06-03 K. S. Babu , Garv Chauhan , P. S. Bhupal Dev

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…

High Energy Physics - Phenomenology · Physics 2021-07-20 Antonio Capolupo , Salvatore Marco Giampaolo , Aniello Quaranta

We study the effect of coherent and incoherent broadening on neutrino oscillations both in vacuum and in the presence of matter (the MSW effect). We show under very general assumptions that it is not possible to distinguish experimentally…

High Energy Physics - Phenomenology · Physics 2009-10-28 Ken Kiers , Shmuel Nussinov , Nathan Weiss

We point out that for solar neutrino oscillations with the mass-squared difference of Delta m^2 ~ 10^-10 - 10^-9 eV^2, traditionally known as ``vacuum oscillation'' range, the solar matter effects are non-negligible, particularly for the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Alexander Friedland

The distortions in the thermal energy spectra for neutrinos produced in a supernova when a resonant oscillation, MSW effect, occurs are determined. In order to show this effect for some relevant and representative examples of unified gauge…

High Energy Physics - Phenomenology · Physics 2008-11-26 F. Buccella , S. Esposito , C. Gualdi , G. Miele

The presence of light (m_a ~ 10^-6 ev) scalar fields in the early universe can modify the cosmology of neutrinos considerably by allowing their masses to vary on cosmological times. In this paper, we consider the effect of Planck-suppressed…

High Energy Physics - Phenomenology · Physics 2009-11-11 Neal Weiner , Kathryn Zurek

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Yu. Smirnov

The MSW or vacuum oscillation solution of the solar neutrino problem can be reconciled with possible existence of the $(\beta\beta)_{0\nu}$ decay with a half-life corresponding to an effective Majorana mass of the electron neutrino…

High Energy Physics - Phenomenology · Physics 2009-10-22 S. T. Petcov , A. Yu. Smirnov

Assuming three-neutrino mixing, we study the capabilities of very long baseline neutrino oscillation experiments to verify and test the MSW effect and to measure the lepton mixing angle theta_13. We suppose that intense neutrino and…

High Energy Physics - Phenomenology · Physics 2014-11-17 M. Freund , M. Lindner , S. T. Petcov , A. Romanino

We investigate a model where neutrinos are strongly coupled to a new, light scalar field. In this model neutrinos annihilate as soon as they become non-relativistic in the early universe, and a non-zero neutrino mass has a marginal effect…

Astrophysics · Physics 2010-12-09 Steen Hannestad

We consider neutrinos with varying masses which arise in scenarios relating neutrino masses to the dark energy density in the universe. We point out that the neutrino mass variation can lead to level crossing and thus a cosmo MSW effect,…

Astrophysics · Physics 2008-11-26 Pham Quang Hung , Heinrich Päs
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