2019
DOI: 10.1134/s1063776119120197
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The Solar Neutrino Problem as Evidence of New Interaction

Abstract: A new concept is proposed to solve the solar neutrino problem, that is based on a hypothesis about the existence of a new interaction of electron neutrinos with nucleons mediated by massless pseudoscalar bosons. At every collision of a neutrino with nucleons of the Sun, its handedness changes from left to right and vice versa, and its energy decreases. The postulated hypothesis, having only one free parameter, provides a good agreement between the calculated and experimental characteristics of all five observe… Show more

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Cited by 3 publications
(3 citation statements)
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“…For a fixed energy from this interval, the oscillation length of the probability P e (t) has a maximum value at the matter density of the Sun corresponding to the extremal electron density (10). When the neutrino energy increases from 0.827 to 18.8 MeV, the extremal density of matter decreases from 148 to 6.51 g/cm 3 . The oscillation length of the probability P e (t) takes a minimum value at one of the boundary points of the matter density range [0, 148] g/cm 3 .…”
Section: See Eq (3) Abovementioning
confidence: 99%
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“…For a fixed energy from this interval, the oscillation length of the probability P e (t) has a maximum value at the matter density of the Sun corresponding to the extremal electron density (10). When the neutrino energy increases from 0.827 to 18.8 MeV, the extremal density of matter decreases from 148 to 6.51 g/cm 3 . The oscillation length of the probability P e (t) takes a minimum value at one of the boundary points of the matter density range [0, 148] g/cm 3 .…”
Section: See Eq (3) Abovementioning
confidence: 99%
“…When the neutrino energy increases from 0.827 to 18.8 MeV, the extremal density of matter decreases from 148 to 6.51 g/cm 3 . The oscillation length of the probability P e (t) takes a minimum value at one of the boundary points of the matter density range [0, 148] g/cm 3 . At the neutrino energy E = 18.8 MeV, the oscillation length of the probability P e (t) lies in the interval from 134 km to 1028 km, i.e., from 0.000193R 0 to 0.00148R 0 , at which it is equal to L(0) = 968 km at the exit from the Sun.…”
Section: See Eq (3) Abovementioning
confidence: 99%
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