Results 91 to 100 of about 5,641,267 (259)

Testing large non-standard neutrino interactions with arbitrary mediator mass after COHERENT data

open access: yesJournal of High Energy Physics, 2018
A bstractIn the presence of neutrino Non-Standard Interactions (NSI) with matter, the derivation of neutrino parameters from oscillation data must be reconsidered.
P. Denton, Y. Farzan, I. Shoemaker
semanticscholar   +1 more source

Cosmological signatures of interacting neutrinos [PDF]

open access: yesPhysical Review D, 2006
We investigate signatures of neutrino scattering in the Cosmic Microwave Background (CMB) and matter power spectra, and the extent to which present cosmological data can distinguish between a free streaming or tightly coupled fluid of neutrinos. If neutrinos have strong non-standard interactions, for example, through the coupling of neutrinos to a ...
Kris Sigurdson   +3 more
openaire   +5 more sources

Nonstandard neutrino interactions in a modified ν2HDM [PDF]

open access: yesPhysical Review D, 2018
In the traditional neutrinophilic two-Higgs doublet model ($\nu$2HDM), there is no non-standard neutrino interaction (NSI) as the interactions between the Standard Model fermions with neutrinos are negligibly small due to the tiny mixing of the two ...
U. Dey, Newton Nath, Soumya Sadhukhan
semanticscholar   +1 more source

Theory of neutrino slow flavor evolution. Part II. Space-time evolution of linear instabilities

open access: yesJournal of High Energy Physics
Slow flavor evolution (defined as driven by neutrino masses and not necessarily “slow”) is receiving fresh attention in the context of compact astrophysical environments.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj   +1 more source

Impact of right-handed interactions on the propagation of Dirac and Majorana neutrinos in matter

open access: yes, 2007
Dirac and Majorana neutrinos can be distinguished in relativistic neutrino oscillations if new right-handed interactions exist, due to their different propagation in matter. We review how these new interactions affect neutrino oscillation experiments and
A. S. Barabash   +19 more
core   +1 more source

Flavor changing neutrino interactions and CP violation in neutrino oscillations [PDF]

open access: yes, 2002
We investigate the interference effects of non-standard neutrino-matter interactions (NSNI) with the mass-induced neutrino oscillations. The NSNI is composed of flavor-changing neutrino interactions (FCNI) and flavor-diagonal neutrino interactions (FDNI).
Hasuike, T., Hattori, T., Wakaizumi, S.
core   +2 more sources

Non-standard neutrino interactions and low energy experiments

open access: yesJournal of High Energy Physics, 2019
We formulate an Effective Field Theory (EFT) for Non Standard neutrino Interactions (NSI) in elastic scattering with light quarks, leptons, gluons and photons, including all possible operators of dimension 5, 6 and 7.
W. Altmannshofer, M. Tammaro, J. Zupan
semanticscholar   +1 more source

Neutrino masses in a two Higgs doublet model with a U(1) gauge symmetry

open access: yesJournal of High Energy Physics, 2019
General Two Higgs Doublet Models (2HDM) are popular Standard Model extensions but feature flavor changing interactions and lack neutrino masses. We discuss a 2HDM where neutrino masses are generated via type I seesaw and propose an extension where ...
Daniel A. Camargo   +3 more
doaj   +1 more source

Bounds on non-standard interactions of neutrinos from IceCube DeepCore data

open access: yesJournal of High Energy Physics, 2020
New physics in neutrino sector can reveal itself via non-standard neutrino in- teractions which can result in modification of the standard picture of neutrino propagation in matter.
S.V. Demidov
doaj   +1 more source

High-energy constraints from low-energy neutrino non-standard interactions

open access: yes, 2020
Many scenarios of new physics predict the existence of neutrino Non-Standard Interactions, new vector contact interactions between neutrinos and first generation fermions beyond the Standard Model.
Terol-Calvo, Jorge   +2 more
core   +1 more source

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