Results 121 to 130 of about 243,227 (257)
, 2009 For the electroweak interactions, the massive neutrino perturbative kinematical procedure is developed in the massive neutrino Fock space. This yields the dominant Lorentz invariant Standard Model mass-less flavor neutrino cross-sections as well as the ...
+12 more
core +1 more source
Neutrino masses and neutrino mixing
Nuclear Physics B - Proceedings Supplements, 2006 We review the current (summer 2005) status of neutrino mass and mixing parameters, as emerging from a phenomenological analysis of world neutrino oscillation and non-oscillation data, performed within the standard three-neutrino mixing framework.
Antonio Marrone +4 more
openaire +3 more sources
Substantia, 2017 Joseph Weber, form Maryland University, was a pioneer in the experimental research of gravitational waves and neutrinos. Today these two techniques are very promising for astronomical observation, since will allow to observe astrophysical phenomena under
Stefano Gottardo
doaj +1 more source
A Soil Scientist Goes to Washington: Navigating the Path to National Science Leadership
AGU Advances, Volume 6, Issue 3, June 2025.
Asmeret Asefaw Berhe
wiley +1 more source
Pacific Ocean Neutrino Experiment
UniverseFollowing the breakthrough discoveries of very-high-energy neutrinos of astrophysical origin by IceCube, a new field of research, neutrino astronomy, was established in the previous decade.
Paweł Malecki
doaj +1 more source
Compreendendo a oscilação dos neutrinos
Revista Brasileira de Ensino de FísicaEste trabalho é uma introdução ao modelo da oscilação de neutrinos para estudantes de física. Apresentamos o modelo de mistura de neutrinos baseado no conceito de superposição de estados. Em particular, consideraremos o caso onde os neutrinos se propagam
Gustavo do A. Valdiviesso +1 more
doaj +1 more source
On Cooling of Neutron Stars with a Stiff Equation of State Including Hyperons
Universe, 2018 Exploiting a stiff equation of state of the relativistic mean-field model MKVORH ϕ with σ -scaled hadron effective masses and couplings, including hyperons, we demonstrate that the existing neutron-star cooling data can be appropriately ...
Hovik Grigorian +3 more
doaj +1 more source
Neutrino clustering in growing neutrino quintessence
Physics Letters B, 2008 A growing neutrino mass can stop the dynamical evolution of a dark energy scalar field, thus explaining the 'why now' problem. We show that such models lead to a substantial neutrino clustering on the scales of superclusters. Nonlinear neutrino lumps form at redshift z \sim 1 and could partially drag the clustering of dark matter.
Christof Wetterich +3 more
openaire +3 more sources