2020
DOI: 10.3103/s106287382003003x
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Supernonradiative States, Neutrinos, and Higgs Bosons in Fractal Quantum Systems

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Cited by 6 publications
(6 citation statements)
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“…Using the parameters hL = 0.000118617 from [4,5], N hS from ( 21), we find the value N L3 = 119.5712542 and the estimate of the distance L 3 = 119.5712542 au. To estimate the distance L 1 (inside the heliosphere for L 1 < L 2 ), we use the characteristic distances L μe , L μμ , L μτ for e, μ, τ -leptons, respectively, determined by the expressions…”
Section: Solar Wind and Heliopausementioning
confidence: 97%
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“…Using the parameters hL = 0.000118617 from [4,5], N hS from ( 21), we find the value N L3 = 119.5712542 and the estimate of the distance L 3 = 119.5712542 au. To estimate the distance L 1 (inside the heliosphere for L 1 < L 2 ), we use the characteristic distances L μe , L μμ , L μτ for e, μ, τ -leptons, respectively, determined by the expressions…”
Section: Solar Wind and Heliopausementioning
confidence: 97%
“…The compound of the solar wind may include active nanoobjects [4][5][6][7] and femtoobjects. Based on the results of [1,2,[4][5][6][7], we introduce the main parameters ξ 2 p , A0 , r p of a model femtoobject (…”
Section: Description Of Model Femtoobjectmentioning
confidence: 99%
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