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Related papers: Beyond the MSW effect: Neutrinos in a dense medium

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Fermions act as sources of spacetime torsion. However, this torsion is non-dynamical and can be eliminated using its equations of motion. The resulting theory features an effective four-fermion interaction in a torsion-free background.…

High Energy Physics - Phenomenology · Physics 2025-12-03 Riya Barick , Amitabha Lahiri

Neutrinos play a critical role of transporting energy and changing the lepton density within core-collapse supernovae and neutron star mergers. The quantum kinetic equations (QKEs) combine the effects of neutrino-matter interactions treated…

High Energy Astrophysical Phenomena · Physics 2024-09-13 Sherwood A. Richers , Gail C. McLaughlin , James P. Kneller , Alexey Vlasenko

We study the oscillations and conversions of relativistic neutrinos propagating in matter of variable density using the wave packet formalism. We show how the oscillation and coherence lengths are modified in comparison with the case of…

High Energy Physics - Phenomenology · Physics 2011-07-19 J. T. Peltoniemi , V. Sipilainen

The neutrino oscillation enhancement in the Earth-type medium mantle - core - mantle is discussed. It is noted that the total conversion is possible both for a resonant matter density and a nonresonant one. A useful parameterization, for…

High Energy Physics - Phenomenology · Physics 2007-05-23 M. V. Chizhov

We consider a class of theories in which neutrino masses depend significantly on environment, as a result of interactions with the dark sector. Such theories of mass varying neutrinos (MaVaNs) were recently introduced to explain the origin…

High Energy Physics - Phenomenology · Physics 2009-11-10 David B. Kaplan , Ann E. Nelson , Neal Weiner

We investigate the $\nu_e \to \nu_{\mu}$ oscillation in the framework of three generations when neutrinos pass through the earth. The oscillation probability is represented by the form, $P(\nu_e \to \nu_\mu)=A\cos \delta+B\sin \delta+C$ in…

High Energy Physics - Phenomenology · Physics 2009-11-10 Keiichi Kimura , Akira Takamura , Hidekazu Yokomakura

The flavor conversion of supernova neutrinos can lead to observable signatures related to the unknown neutrino parameters. As one of the determinants in dictating the efficiency of resonant flavor conversion, the local density profile near…

High Energy Physics - Phenomenology · Physics 2008-11-26 Shao-Hsuan Chiu

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

Neutrinos, due to their weakly interacting nature, provide us with a unique opportunity to test foundations of quantum mechanics over macroscopic distances. There has been considerable theoretical and experimental interest in examining the…

High Energy Physics - Phenomenology · Physics 2021-12-28 Sheeba Shafaq , Tanmay Kushwaha , Poonam Mehta

In this paper, we study the effect of conversion of super-light sterile neutrino (SLSN) to electron neutrino in matter like that of the Earth. In the Sun the resonance conversion between SLSN and electron neutrino via the neutral current is…

High Energy Physics - Phenomenology · Physics 2016-08-01 P. C. Divari , J. D. Vergados

We review neutrino oscillation physics, including the determination of mass splittings and mixings from current solar, atmospheric, reactor and accelerator neutrino data. A brief discussion is given of cosmological and astrophysical…

High Energy Physics - Phenomenology · Physics 2009-09-17 S. Pakvasa , J. W. F. Valle

We discuss a novel effect in neutrinoless double beta (0{\nu}{\beta}{\beta}) decay related with the fact that its underlying mechanisms take place in the nuclear matter environment. We study the neutrino exchange mechanism and demonstrate…

High Energy Physics - Phenomenology · Physics 2014-04-23 S. Kovalenko , M. I. Krivoruchenko , F. Simkovic

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

Even the elusive neutrinos are trapped in matter, albeit transiently, in several astrophysical circumstances. Their interactions with the ambient matter not only reveal the properties of such exotic matter itself, but also shed light on the…

Astrophysics · Physics 2009-11-06 M. Prakash , J. M. Lattimer , R. F. Sawyer , R. R. Volkas

A comprehensive formalism for the description of neutrino oscillations in the Earth in a general scheme with three massive neutrinos and the mass hierarchy m_1<<m_2<<m_3 is presented. Using this formalism, which is valid both in vacuum and…

High Energy Physics - Phenomenology · Physics 2011-07-19 C. Giunti , C. W. Kim , M. Monteno

The possibility is explored that neutrino condensates, possible candidates for the explanation of very massive objects in galactic centers, could act as background for the Mikheyev-Smirnov-Wolfeinstein mechanism responsible of neutrino…

Astrophysics · Physics 2008-11-26 S. Capozziello , G. Iovane , G. Lambiase

In this brief review, I discuss the new physics unveiled by neutrino oscillation experiments over the past several years, and discuss several attempts at understanding the mechanism behind neutrino masses and lepton mixing. It is fair to…

High Energy Physics - Phenomenology · Physics 2009-11-11 Andre de Gouvea

The historical discovery of neutrino oscillations using solar and atmospheric neutrinos, and subsequent accelerator and reactor studies, has brought neutrino physics to the precision era. We note that CP effects in oscillation phenomena…

High Energy Physics - Phenomenology · Physics 2016-06-22 O. G. Miranda , J. W. F. Valle

In this work, we calculate expression for the potential due to neutrino-(anti)neutrino forward scattering at low energies ($E<<m_{Z^0}$) for ultra-relativistic massive neutrinos ($E>>m_{\nu}$), a representative regime within astrophysical…

High Energy Physics - Phenomenology · Physics 2022-04-07 Pedro Dedin Neto , Ernesto Kemp

Neutrino propagation in space-time is not constrained to be unitary if very light states - lighter than the active neutrinos - exist into which neutrinos may decay. If this is the case, neutrino flavor-change is governed by a handful of…

High Energy Physics - Phenomenology · Physics 2015-02-13 Jeffrey M. Berryman , André de Gouvêa , Daniel Hernández , Roberto L. N. Oliveira