Neutrino mass and mixing with discrete symmetry

SF King, C Luhn - Reports on Progress in Physics, 2013 - iopscience.iop.org
This is a review paper about neutrino mass and mixing and flavour model building strategies
based on discrete family symmetry. After a pedagogical introduction and overview of the …

Neutrino oscillations and non-standard interactions

Y Farzan, M Tórtola - Frontiers in Physics, 2018 - frontiersin.org
Current neutrino experiments are measuring the neutrino mixing parameters with an
unprecedented accuracy. The upcoming generation of neutrino experiments will be …

Five-year wilkinson microwave anisotropy probe* observations: cosmological interpretation

E Komatsu, J Dunkley, MR Nolta… - The Astrophysical …, 2009 - iopscience.iop.org
ABSTRACT The Wilkinson Microwave Anisotropy Probe (WMAP) 5-year data provide
stringent limits on deviations from the minimal, six-parameter Λ cold dark matter model. We …

Improved measurement of neutrino oscillation parameters by the NOvA experiment

MA Acero, P Adamson, L Aliaga, N Anfimov… - Physical Review D, 2022 - APS
We present new ν μ→ ν e, ν μ→ ν μ, ν¯ μ→ ν¯ e, and ν¯ μ→ ν¯ μ oscillation measurements
by the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over the …

A facility to Search for Hidden Particles at the CERN SPS: the SHiP physics case

S Alekhin, W Altmannshofer, T Asaka… - Reports on progress …, 2016 - iopscience.iop.org
This paper describes the physics case for a new fixed target facility at CERN SPS. The SHiP
(search for hidden particles) experiment is intended to hunt for new physics in the largely …

The GENIE neutrino monte carlo generator

C Andreopoulos, A Bell, D Bhattacharya… - Nuclear Instruments and …, 2010 - Elsevier
GENIE [1] is a new neutrino event generator for the experimental neutrino physics
community. The goal of the project is to develop a 'canonical'neutrino interaction physics …

First measurement of neutrino oscillation parameters using neutrinos and antineutrinos by NOvA

MA Acero, P Adamson, L Aliaga, T Alion… - Physical review …, 2019 - APS
The NOvA experiment has seen a 4.4 σ signal of ν¯ e appearance in a 2 GeV ν¯ μ beam at a
distance of 810 km. Using 12.33× 10 20 protons on target delivered to the Fermilab NuMI …

[BOOK][B] Introduction to the theory of the early universe: Cosmological perturbations and inflationary theory

DS Gorbunov, VA Rubakov - 2011 - books.google.com
This book accompanies another book by the same authors, Introduction to the Theory of the
Early Universe: Hot Big Bang Theory and presents the theory of the evolution of density …

From the trees to the forest: a review of radiative neutrino mass models

Y Cai, J Herrero García, MA Schmidt, A Vicente… - Frontiers in …, 2017 - frontiersin.org
A plausible explanation for the lightness of neutrino masses is that neutrinos are massless at
tree level, with their mass (typically Majorana) being generated radiatively at one or more …

Flavor structures of charged fermions and massive neutrinos

Z **ng - Physics Reports, 2020 - Elsevier
Most of the free parameters in the Standard Model (SM)—a quantum field theory which has
successfully elucidated the behaviors of strong, weak and electromagnetic interactions of all …