Results 71 to 80 of about 59,601 (214)

High energy neutrino signals of four neutrino mixing [PDF]

open access: yesPhysical Review D, 2001
version accepted for publication in Phys.
Dutta, Sharada Iyer   +2 more
openaire   +2 more sources

Quantum GraviElectro Dynamics

open access: yesAnnalen der Physik, Volume 538, Issue 1, January 2026.
The BRST invariant Lagrangian of the gravitationally interacting U(1)$U(1)$ gauge theory, namely the Quantum GraviElectro Dynamics (QGED). The Yan–Mills theory with the Hilbert–Einstein gravitational Lagrangian, namely the Yang–Mills–Utiyama (YMU) theory, is defined and quantised using the standard procedure. The theory is perturbatively renormalisable,
Yoshimasa Kurihara
wiley   +1 more source

Testing sterile neutrino mixing with present and future solar neutrino data

open access: yesEuropean Physical Journal C: Particles and Fields, 2022
We investigate the sensitivity of solar neutrino data to mixing of sterile neutrinos with masses $$\gtrsim $$ ≳  eV. For current data, we perform a Feldman–Cousins analysis to derive a robust limit on the sterile neutrino mixing. The solar neutrino limit
Kim Goldhagen   +3 more
doaj   +1 more source

A Renormalizable Neutrino Mass Model With (Z2 × Z4)⋊Z2(II) Symmetry

open access: yesAdvances in High Energy Physics, Volume 2026, Issue 1, 2026.
In this work, a renormalizable neutrino mass model based on (Z2 × Z4)⋊Z2 (II) symmetry is proposed for the modification of the μ − τ reflection symmetry. The hierarchies of lepton masses can be naturally realized, and the lepton mixing is addressed.
V. V. Vien   +3 more
wiley   +1 more source

Large mixing angles for neutrinos from infrared fixed points

open access: yes, 2003
Radiative amplification of neutrino mixing angles may explain the large values required by solar and atmospheric neutrino oscillations. Implementation of such mechanism in the Standard Model and many of its extensions (including the Minimal ...
Casas, J. A.   +2 more
core   +1 more source

Neutrino masses from operator mixing [PDF]

open access: yes, 2001
We show that in theories that reduce, at the Fermi scale, to an extension of the standard model with two doublets, there can be additional dimension five operators giving rise to neutrino masses.
A. Santamaria   +31 more
core   +3 more sources

Neutrino Mixing: Theoretical Overview

open access: yesIl Nuovo Cimento C, 2013
We present a concise review of the recent important experimental developments on neutrino mixing (hints for sterile neutrinos, large $ _{13}$, possible non maximal $ _{23}$, approaching sensitivity on $ _{CP}$) and their implications on models of neutrino mixing. The new data disfavour many models but the surviving ones still span a wide range going
openaire   +3 more sources

Search for heavy neutrinos mixing with tau neutrinos [PDF]

open access: yesPhysics Letters B, 2001
We report on a search for heavy neutrinos ($\nus$) produced in the decay $D_s\to \nus$ at the SPS proton target followed by the decay $\nudecay$ in the NOMAD detector. Both decays are expected to occur if $\nus$ is a component of $ _ $.\ From the analysis of the data collected during the 1996-1998 runs with $4.1\times10^{19}$ protons on target, a ...
Astier P   +147 more
openaire   +5 more sources

A Superalgebra Within: Representations of Lightest Standard Model Particles Form a Z25$\mathbb {Z}_2^5$‐Graded Algebra

open access: yesAnnalen der Physik, Volume 537, Issue 12, December 2025.
 A set of particle representations, familiar from the Standard Model, collectively form a superalgebra. Those representations mirroring the behaviour of the Standard Model's gauge bosons, and three generations of fermions, are each included in this algebra, with exception only to those representations involving the top quark.
N. Furey
wiley   +1 more source

Constraints on Exotic Mixing of Three Neutrinos [PDF]

open access: yes, 1999
Exotic explanations are considered for atmospheric neutrino observations. Our analysis includes matter effects and the mixing of all three neutrinos under the simplifying assumption of only one relevant mixing scale. Constraints from accelerator, reactor
A. Halprin   +51 more
core   +3 more sources

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