dorsal/arxiv
View SchemaAre There "Neutrino Flavors"? : More on the Equation H = mv^2
| Authors | Ezzat G. Bakhoum |
|---|---|
| Categories | |
| ArXiv ID | physics/0302095 |
| URL | https://arxiv.org/abs/physics/0302095 |
Abstract
In a recent work by the author it was demonstrated that the "neutrino" that is currently being detected in solar reactions (and possibly in other high energy nuclear reactions) is not Pauli's particle; as it became clear that such a particle is an unnecessary proposition in explaining the beta-decay reaction. In addition, it became obvious that concepts such as "flavor oscillations" of the solar neutrinos are superfluous. In this paper it is further demonstrated that if certain key experiments of the past are reinterpreted in view of the total energy equation H=mv^2, then the principle of the existence of different neutrino "flavors" is itself very questionable.
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"abstract": "In a recent work by the author it was demonstrated that the \"neutrino\" that\nis currently being detected in solar reactions (and possibly in other high\nenergy nuclear reactions) is not Pauli\u0027s particle; as it became clear that such\na particle is an unnecessary proposition in explaining the beta-decay reaction.\nIn addition, it became obvious that concepts such as \"flavor oscillations\" of\nthe solar neutrinos are superfluous. In this paper it is further demonstrated\nthat if certain key experiments of the past are reinterpreted in view of the\ntotal energy equation H=mv^2, then the principle of the existence of different\nneutrino \"flavors\" is itself very questionable.",
"arxiv_id": "physics/0302095",
"authors": [
"Ezzat G. Bakhoum"
],
"categories": [
"physics.gen-ph"
],
"title": "Are There \"Neutrino Flavors\"? : More on the Equation H = mv^2",
"url": "https://arxiv.org/abs/physics/0302095"
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