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arXiv 1502.03262hep-phastro-ph.SRhep-exnucl-th
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半弱相互作用假说与太阳中微子实验

Hypothesis about semi-weak interaction and experiments with solar neutrinos

L. M. Slad

备注：
12 pages. The main material is contained in JETP 129 (2019) 973
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摘要：

提出了一个解决太阳中微子问题的新概念，即基于电子中微子与核子之间存在无质量赝标玻色子介导的半弱相互作用的假设。由于一个太阳中微子与太阳核子的大约10次碰撞，地球表面的左手和右手太阳中微子的通量近似相等，并且它们的光谱与产生时刻的光谱相比发生了变化。假设的模型与一个自由参数提供了一个很好的协议与太阳中微子的过程：${}^{37}{\rm Cl} \rightarrow {}^{37}{\rm Ar}$，${}^{71}{\rm Ga} \rightarrow {}^{71}{\rm Ge}$，$ν_{e} e^{-}\rightarrow ν_{e} e^{-}$，和$ν_{e}D \rightarrow e^{-}pp$的计算和实验之间的特性。

英文摘要：

A new concept is proposed to solve the solar neutrino problem, that is based on a hypothesis about the existence of semi-weak interaction of electron neutrinos with nucleons mediated by massless pseudoscalar bosons. Owing to about 10 collisions of a solar neutrino with nucleons of the Sun, the fluxes of left- and right-handed solar neutrinos at the Earth surface are approximately equal, and their spectrum is changed in comparison with the one at the production moment. The postulated model with one free parameter provides a good agreement between the calculated and experimental characteristics of the processes with solar neutrinos: ${}^{37}{\rm Cl} \rightarrow {}^{37}{\rm Ar}$, ${}^{71}{\rm Ga} \rightarrow {}^{71}{\rm Ge}$, $ν_{e} e^{-}\rightarrow ν_{e} e^{-}$, and $ν_{e}D \rightarrow e^{-}pp$.

机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。

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