论文标题
中微子在太阳中的布朗运动[关于与太阳核子的中微子碰撞的分布]
Brownian motion of neutrinos in the Sun [On the distribution of collisions of a neutrino with nucleons of the Sun]
论文作者
论文摘要
当根据由无质量伪统一的玻色子携带的电子中微子和核子之间存在新相互作用的假设解决太阳中微子问题时，有必要找到短期布朗尼在太阳中的布朗尼运动的后果。早些时候，我们通过与太阳核的有效碰撞数量传递了这些后果，假设左手和右手太阳中微子的地球附近的通量相等。在本文中，我们通过使用一个自由参数的碰撞测试几何分布来分析上述后果的转移。该分布在所有五个观测到的太阳中微子的过程中提供了良好的一致性和实验结果之间的一致性，而左和右中微子的地球附近的通量比等于0.516：0.484。以这样的比率，再次证实了中微子与核子的有效数量碰撞的方法的可接受性。
When solving the solar neutrino problem on the basis of the hypothesis of the existence of a new interaction between electron neutrinos and nucleons, carried by a massless pseudoscalar boson, it becomes necessary to find the consequences of the short-term Brownian motion of neutrinos in the Sun. Earlier, we transmitted these consequences by the effective number of collisions of a neutrino with nucleons of the Sun, assuming the equality of fluxes near the Earth of left- and right-handed solar neutrinos. In this paper, we analyze the transfer of the mentioned consequences by a test geometric distribution of collisions with one free parameter. This distribution provides good agreement between theoretical and experimental results for all five observed processes with solar neutrinos, while it gives the ratio of fluxes near the Earth of left- and right-handed neutrinos equal to 0.516:0.484. With such a ratio, the acceptability of the method of the effective number of collisions of a neutrino with nucleons is again confirmed.
