Results 31 to 40 of about 41,366 (209)

A road map to solar neutrino fluxes, neutrino oscillation parameters, and tests for new physics [PDF]

open access: yes, 2003
We analyze all available solar and related reactor neutrino experiments, as well as simulated future 7Be, p-p, pep, and ^8B solar neutrino experiments.
Bahcall, John N., Pena-Garay, Carlos
core   +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 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

Non-standard interactions of solar neutrinos in dark matter experiments

open access: yesPhysics Letters B, 2017
We show that non-standard neutrino interactions (NSI) can be probed in future direct dark matter detection experiments through both elastic neutrino-electron scattering and coherent neutrino-nucleus scattering. We show NSI can increase the event rate due
Bhaskar Dutta   +3 more
doaj   +1 more source

Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II

open access: yesJournal of High Energy Physics, 2020
The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics
The Borexino collaboration   +106 more
doaj   +1 more source

Solar neutrino with Borexino: results and perspectives [PDF]

open access: yes, 2014
Borexino is a unique detector able to perform measurement of solar neutrinos fluxes in the energy region around 1 MeV or below due to its low level of radioactive background. It was constructed at the LNGS underground laboratory with a goal of solar $^{7}
Bellini, G.   +89 more
core   +3 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

Solar Neutrinos with Three Flavor Mixings [PDF]

open access: yes, 1992
The recent 71Ga solar neutrino observation is combined with the 37Cl and Kamiokande-II observations in an analysis for neutrino masses and mixings.
A.I. Abazov   +34 more
core   +3 more sources

Solar neutrino spectroscopy [PDF]

open access: yesPhysics Reports, 2017
More than forty years after the first detection of neutrinos from the Sun, the spectroscopy of solar neutrinos has proven to be an on-going success story. The long-standing puzzle about the observed solar neutrino deficit has been resolved by the discovery of neutrino flavor oscillations.
openaire   +2 more sources

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

Home - About - Disclaimer - Privacy