Results 61 to 70 of about 1,187,743 (285)

The Simplest Resonant Spin--Flavour Solution to the Solar Neutrino Problem [PDF]

open access: yes, 2000
We re-analyse the resonant spin-flavour (RSF) solutions to the solar neutrino problem in the framework of analytic solutions to the solar magneto-hydrodynamics (MHD) equations.
Akhmedov   +57 more
core   +2 more sources

Solar Neutrinos

open access: yesLa Rivista Del Nuovo Cimento Series 3, 1993
19 pages, 2 figures (available on request), Coral Gables talk, UPR ...
openaire   +5 more sources

Solar Neutrinos Spectroscopy with Borexino Phase-II

open access: yesUniverse, 2018
Solar neutrinos have played a central role in the discovery of the neutrino oscillation mechanism. They still are proving to be a unique tool to help investigate the fusion reactions that power stars and further probe basic neutrino properties.
Lino Miramonti   +109 more
doaj   +1 more source

Solar ν ¯ e $$ {\overline{\nu}}_e $$ flux: revisiting bounds on neutrino magnetic moments and solar magnetic field

open access: yesJournal of High Energy Physics, 2022
The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP).
Evgeny Akhmedov, Pablo Martínez-Miravé
doaj   +1 more source

NEUTRINO-DRIVEN EXPLOSION OF A 20 SOLAR-MASS STAR IN THREE DIMENSIONS ENABLED BY STRANGE-QUARK CONTRIBUTIONS TO NEUTRINO–NUCLEON SCATTERING [PDF]

open access: yes, 2015
Interactions with neutrons and protons play a crucial role for the neutrino opacity of matter in the supernova core. Their current implementation in many simulation codes, however, is rather schematic and ignores not only modifications for the correlated
T. Melson   +5 more
semanticscholar   +1 more source

Helioseismology and solar neutrinos [PDF]

open access: yesSolar Neutrinos, 2019
The studies of solar neutrinos and helioseismology have been closely intertwined since the first neutrino experiment and the first observations of solar oscillations in the sixties. Early detailed helioseismic analyses provided strong support for the standard solar model and hence a clear indication that the solution to the discrepancy between the ...
openaire   +6 more sources

Combined Effect of NSI and SFP on Solar Electron Neutrino Oscillation

open access: yesAdvances in High Energy Physics, 2016
The combined effect of spin-flavor precession (SFP) and the nonstandard neutrino interaction (NSI) on the survival probability of solar electron neutrinos (assumed to be Dirac particles) is examined for various values of ϵ11, ϵ12, and μB.
Deniz Yilmaz
doaj   +1 more source

Model Independent Information On Solar Neutrino Oscillations [PDF]

open access: yes, 2001
We present the results of a Bayesian analysis of solar neutrino data in terms of nu_e->nu_{mu,tau} oscillations, independent from the Standard Solar Model predictions for the solar neutrino fluxes. We show that such a model independent analysis allows to
A. Bandyopadhyay   +70 more
core   +2 more sources

Solar models and solar neutrino oscillations [PDF]

open access: yes, 2004
We provide a summary of the current knowledge, theoretical and experimental, of solar neutrino fluxes and of the masses and mixing angles that characterize solar neutrino oscillations.
  +32 more
core   +5 more sources

Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation [PDF]

open access: yes, 2015
A comprehensive study on the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande water Cherenkov detector is presented. The energy and azimuthal spectra of the atmospheric νe and νµ fluxes are measured.
K. Okumura
semanticscholar   +1 more source

Home - About - Disclaimer - Privacy