Results 61 to 70 of about 1,199,141 (307)

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

Frontier of Understanding Earth's Dynamics

open access: yes, 2023
Perspectives of Earth and Space Scientists, Volume 4, Issue 1, December 2023.
Hiroko Watanabe   +4 more
wiley   +1 more source

7Be solar neutrino measurement with KamLAND [PDF]

open access: yes, 2014
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV ^7Be solar neutrinos based on a 165.4 kt d exposure of KamLAND. The observed rate is 582±94(kt d)^(−1), which corresponds to an 862-keV Be7 solar neutrino flux of (3.26±0.
A. Gando   +70 more
semanticscholar   +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

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

Shedding light on LMA-dark solar neutrino solution by medium baseline reactor experiments: JUNO and RENO-50 [PDF]

open access: yes, 2014
A bstractIn the presence of Non-Standard neutral current Interactions (NSI) a new solution to solar neutrino anomaly with cos 2θ12 < 0 appears. We investigate how this solution can be tested by upcoming intermediate baseline reactor experiments, JUNO and
P. Bakhti, Y. Farzan
semanticscholar   +1 more source

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

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

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 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

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