Results 41 to 50 of about 35,741 (202)

Solar neutrinos and neutrino physics [PDF]

open access: yesThe European Physical Journal A, 2016
Solar neutrino studies triggered and largely motivated the major developmentsin neutrino physics in the last 50 years. Theory of neutrino propagation indifferent media with matter and fields has been elaborated. It includesoscillations in vacuum and matter, resonance flavor conversion and resonanceoscillations, spin and spin-flavor precession, etc. LMA
Maltoni, M.   +1 more
openaire   +4 more sources

ecCNO solar neutrinos: A challenge for gigantic ultra-pure liquid scintillator detectors

open access: yesPhysics Letters B, 2015
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer as ecCNO neutrinos, are not usually considered in solar neutrino analysis since the expected fluxes are extremely low.
F.L. Villante
doaj   +1 more source

Doublet-Singlet Oscillations and Dark Matter Neutrinos [PDF]

open access: yes, 1996
We examine the `singlet majoron model' first introduced by Chikashige, Mohapatra and Peccei as a simple extension of the standard model with massive Majorana neutrinos.
Okada, Nobuchika
core   +2 more sources

New results on solar neutrino fluxes from 192 days of Borexino data

open access: yes, 2008
We report the direct measurement of the ^7Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso.
A. Brigatti   +138 more
core   +3 more sources

Day-Night and Energy Dependence of MSW Solar Neutrinos for Maximal Mixing [PDF]

open access: yes, 1999
It has been stated in the literature that the case of maximal mixing angle for \nu_e leads to no day-night effect for solar neutrinos and an energy independent flux suppression of 1/2.
Guth, Alan H.   +2 more
core   +3 more sources

A potential test of the CP properties and Majorana nature of neutrinos [PDF]

open access: yes, 1999
The scattering of solar neutrinos on electrons may reveal their CP properties, which are particularly sensitive to their Majorana nature. The cross section is sensitive to the neutrino dipole moments through an interference of electro-magnetic and weak ...
Akhmedov   +24 more
core   +3 more sources

Beyond tree level with solar neutrinos: Towards measuring the flavor composition and CP violation

open access: yesPhysics Letters B, 2023
After being produced as electron neutrinos (νe), solar neutrinos partially change their flavor to νμ and ντ en route to Earth. Although the flavor ratio of the νe flux to the total flux has been well measured, the νμ:ντ composition has not yet been ...
Vedran Brdar, Xun-Jie Xu
doaj   +1 more source

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 neutrino detection sensitivity in DARWIN via electron scattering

open access: yesEuropean Physical Journal C: Particles and Fields, 2020
We detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp, $$^7$$ 7 Be, $$^{13 ...
DARWIN Collaboration   +166 more
doaj   +1 more source

Solar neutrino data, solar model uncertainties and neutrino oscillations [PDF]

open access: yesPhysics Letters B, 1993
We incorporate all existing solar neutrino flux measurements and take solar model flux uncertainties into account in deriving global fits to parameter space for the MSW and vacuum solutions of the solar neutrino problem.
Krauss, Lawrence M.   +2 more
openaire   +2 more sources

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