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Athar, M.S., Barwick, S.W., Brunner, T., Cao, J., Danilov, M., Inoue, K., Kajita, T., Kowalski, M., Lindner, M., Long, K.R., Palanque-Delabrouille, N., Rodejohann, W., Schellman, H., Scholberg, R., Seo, S.H., Smith, N.J.T., Winter, W., Zeller, G.P. and Zukanovich Funchal, R. (2022) Status and Perspectives of Neutrino Physics. Progress in Particle and Nuclear Physics, 124, Article ID: 103947.
https://doi.org/10.1016/j.ppnp.2022.103947
has been cited by the following article:
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TITLE:
Direct Derivation of the Neutrino Mass
AUTHORS:
Volodymyr Krasnoholovets
KEYWORDS:
Charge, Inerton, Mass Defect, Monopole, Neutrino, Space, Tessellattice
JOURNAL NAME:
Journal of High Energy Physics, Gravitation and Cosmology,
Vol.10 No.2,
March
29,
2024
ABSTRACT: In this paper, the submicroscopic deterministic concept developed by the author is applied to the problem of the neutrino mass. A particle appears from space considered as a mathematical lattice of primary topological balls, and induces a deformation coat in its surrounding. The principles of the interaction of particles with space and through space between themselves are considered in detail. The approach states that real quarks possess only an integer charge (±e) and when moving they periodically change to the monopole state (?g) and hence, canonical particles are dynamic dyons. A neutrino emerges as a squeezed quark when it is in a monopole state, or in other words, the quark monopole state (a bubble in the tessellattice) is transferred to the appropriate lepton monopole state (a speck in the tessellattice). The self-mass (a “rest” mass) for each neutrino flavour is calculated. The calculated value of the self-mass for the electron anti-neutrino is 1.22873978 × 10-36 kg = 0.68927247 eV/c2. The concept of neutrino oscillations is revised, and another postulation is proposed, namely, that the transition from lighter to heavier flavors is due to the inelastic scattering of neutrinos on oncoming scatterers. As a result, the neutrino captures the mass defect, becomes heavier, and therefore the transitions Ve?Vμ and Vμ?Vτ occur; thus, the number of light neutrinos decreases in the neutrino flux studied.