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A Short Review on the Latest Neutrinos Mass and Number Constraints from Cosmological Observables
Universe, 2022 We review the neutrino science, focusing on its impact on cosmology along with the latest constraints on its mass and number of species. We also discuss its status as a possible solution to some of the recent cosmological tensions, such as the Hubble ...
Ziad Sakr
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Energy and Momentum of Oscillating Neutrinos [PDF]
, 2001 It is shown that Lorentz invariance implies that in general flavor neutrinos in oscillation experiments are superpositions of massive neutrinos with different energies and different momenta.
C. GIUNTI +9 more
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Multimessenger Search for the Sources of Cosmic Rays Using Cosmic Neutrinos
Frontiers in Astronomy and Space Sciences, 2019 After updating the status of the measurements of the cosmic neutrino flux by the IceCube experiment, we summarize the evidence for the first identified source of cosmic rays and speculate on the connection between the two observations.
Francis Halzen, Ali Kheirandish
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Atmospheric leptons, the search for a prompt component [PDF]
, 2013 The flux of high-energy (>GeV) neutrinos consists primarily of those produced by cosmic-ray interactions in the atmosphere. The contribution from extraterrestrial sources is still unknown. Current limits suggest that the observed spectrum is dominated by
Gaisser, Thomas K.
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Annalen der Physik, 2013 The various experiments on neutrino oscillation evidence that neutrinos have indeed non‐zero masses but cannot provide the absolute neutrino mass scale. This scale of neutrino masses is very important for understanding the evolution and the structure formation of the universe as well as for nuclear and particle physics beyond the present Standard Model.
Weinheimer, Christian, Zuber, Kai
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AIP Conference Proceedings, 1966 The predicted capture rate in the Cl37 experiment for detecting solar neutrinos is calculated using the results of recent nuclear experiments and solar-model investigations. It is shown that additional experiments (e.g., with H2, Li7, B11, or ν-e scattering) are necessary to establish the relative contributions of the proton-proton chain and the CNO ...
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Theoretical Search for Gravitational Bound States of Tachyons
Particles, 2022 The mission here is to see if we can find bound states for tachyons in some gravitational environment. That could provide an explanation for the phenomena called Dark Matter. Starting with the standard Schwarzschild metric in General Relativity, which is
Charles Schwartz
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Sterile neutrinos with pseudoscalar self-interactions and cosmology [PDF]
, 2015 Sterile neutrinos in the electronvolt mass range are hinted at by a number of terrestrial neutrino experiments. However, such neutrinos are highly incompatible with data from the Cosmic Microwave Background and large scale structure. This paper discusses
Archidiacono, Maria +3 more
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Ultrahigh Energy Tau Neutrinos [PDF]
, 2005 We study ultrahigh energy astrophysical neutrinos and the contribution of tau neutrinos from neutrino oscillations, relative to the contribution of the other flavors.
Jones, J. +3 more
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Neutrino masses and solar neutrinos [PDF]
Physical Review D, 1992 It has been pointed out by Bahcall and Bethe and others that all solar-neutrino data can be explained by Mikheyev-Smirnov-Wolfenstein oscillations with $m({\ensuremath{\nu}}_{\ensuremath{\mu}})\ensuremath{\sim}{10}^{\ensuremath{-}3}$ eV consistent with ideas of grand unified theories (GUT's).
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