Results 81 to 90 of about 6,622 (234)

Reactor Neutrinos

open access: yesAdvances in High Energy Physics, Volume 2013, Issue 1, 2013., 2013
We review the status and the results of reactor neutrino experiments. Short‐baseline experiments have provided the measurement of the reactor neutrino spectrum, and their interest has been recently revived by the discovery of the reactor antineutrino anomaly, a discrepancy between the reactor neutrino flux state of the art prediction and the ...
Soo-Bong Kim   +3 more
wiley   +1 more source

Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data [PDF]

open access: yes, 2017
A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment.
M. Agostini   +106 more
semanticscholar   +1 more source

Axionlike particles searches in reactor experiments

open access: yesJournal of High Energy Physics, 2021
Reactor neutrino experiments provide a rich environment for the study of axionlike particles (ALPs). Using the intense photon flux produced in the nuclear reactor core, these experiments have the potential to probe ALPs with masses below 10 MeV.
D. Aristizabal Sierra   +3 more
doaj   +1 more source

Light concentrators for Borexino and CTF [PDF]

open access: yesNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2004
Light concentrators for the solar neutrino experiment Borexino and the Counting Test Facility (CTF) have been developed and constructed. They increase the light yield of these detectors by a factor of 2.5 and 8.8, respectively. Technical challenges like long term stability in various media, high reflectivity and radiopurity have been addressed and the ...
Oberauer, L.   +3 more
openaire   +2 more sources

First real–time detection of solar pp neutrinos by Borexino

open access: yesEPJ Web of Conferences, 2016
Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the
Pallavicini M.   +89 more
doaj   +1 more source

New limits on nucleon decays into invisible channels with the BOREXINO Counting Test Facility [PDF]

open access: yes, 2003
The results of background measurements with the second version of the BOREXINO Counting Test Facility (CTF-II), installed in the Gran Sasso Underground Laboratory, were used to obtain limits on the instability of nucleons, bounded in nuclei, for decays ...
't Hooft   +139 more
core   +4 more sources

Borexino: Recent results and future plans

open access: greenPhysics of Particles and Nuclei, 2017
Borexino is continuing to take data and presenting the new results. The most recent Borexino results are discussed and plans for the nearest future are presented.
O. Yu. Smirnov   +95 more
openalex   +6 more sources

Recent results from Borexino

open access: yesJournal of Physics: Conference Series, 2016
We review the solar neutrinos results of Borexino and the limit on the charge conservation obtained in the context of the analysis of the low energy region of the energy spectrum.
Testera, G.   +95 more
openaire   +4 more sources

The geo-neutrinos

open access: yesEPJ Web of Conferences, 2012
The study of the antineutrinos emitted by the radioactive decays in the Earth interior is the only way to investigate how much of the terrestrial heat is produced by these decays and which is their contribution in the various Earth components.
Bellini G.
doaj   +1 more source

Remaining inconsistencies with solar neutrinos: can spin flavour precession provide a clue?

open access: yes, 2009
A few inconsistencies remain after it has been ascertained that LMA is the dominant solution to the solar neutrino problem: why is the SuperKamiokande spectrum flat and why is the Chlorine rate prediction over two standard deviations above the data ...
Bellini G [Borexino Collaboration]   +5 more
core   +1 more source

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