Results 31 to 40 of about 121,866 (201)
The Use of Low Temperature Detectors for Direct Measurements of the Mass of the Electron Neutrino
Advances in High Energy Physics, 2016 Recent years have witnessed many exciting breakthroughs in neutrino physics. The detection of neutrino oscillations has proved that neutrinos are massive particles, but the assessment of their absolute mass scale is still an outstanding challenge in ...
A. Nucciotti
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Tau neutrinos in IceCube, KM3NeT and the Pierre Auger Observatory
SciPost Physics Proceedings, 2019 In 2018, the IceCube collaboration reported evidence for the identification of a blazar as an astrophysical neutrino source. That evidence is briefly summarised here before focusing on the prospects of tau neutrino physics in IceCube, both at high ...
Daan van Eijk
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Neutrino amplitude decomposition: toward observing the atmospheric-solar wave interference
European Physical Journal C: Particles and Fields, 2020 Observation of the interference between the atmospheric and solar oscillation waves with the correct magnitude would provide another manifestation of the three-generation structure of leptons.
Hisakazu Minakata
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Highlights of the TEXONO Research Program on Neutrino and Astroparticle Physics
, 2003 This article reviews the research program and efforts for the TEXONO Collaboration on neutrino and astro-particle physics. The ``flagship'' program is on reactor-based neutrino physics at the Kuo-Sheng (KS) Power Plant in Taiwan.
Li, J., Wong, H. T., Zhou, Z. Y.
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Model Independent Naturalness Bounds on Magnetic Moments of Majorana Neutrinos [PDF]
, 2006 We analyze the implications of neutrino masses for the magnitude of neutrino magnetic moments. By considering electroweak radiative corrections to the neutrino mass, we derive model-independent naturalness upper bounds on neutrino magnetic moments ...
Bell, Nicole F. +4 more
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Sensors, 2023 Neutrinos are difficult to detect because they weakly interact with matter, making their properties least known. The response of the neutrino detector depends on the optical properties of the liquid scintillator (LS).
Na-Ri Kim, Kyung-Kwang Joo, Hyun-Gi Lee
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Neutrino Physics after KamLAND
, 2003 The neutrino anomalies were driving force of the developments in neutrino physics during the last 30 - 35 years. I will consider status of the anomalies after the first KamLAND result. The main questions are "What is left?" and "What is the next?" In the
Smirnov, Alexei Yu.
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Neutrino emission in neutron matter from magnetic moment interactions [PDF]
, 2004 Neutrino emission drives neutron star cooling for the first several hundreds of years after its birth. Given the low energy ($\sim$ keV) nature of this process, one expects very few nonstandard particle physics contributions which could affect this rate.
Charles Gale +10 more
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Journal of High Energy Physics, 2023 Canonical neutrino oscillations arise due to the propagation of three mass eigenstates from production to detection. We aspire to capture, in one simple framework, a broad range of new physics effects on neutrino propagation beyond this canonical picture
Hannah Banks +2 more
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Neutrinos in a Minimal 3-3-1 Model
Frontiers in Physics, 2022 In this work, we present a general review of neutrino physics in the minimal 331 model. New gauge and scalar interactions are present, with violation of both flavor and lepton numbers.
M. M. Guzzo +2 more
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