标题： 广义统计与太阳中微子 显示英文标题

标题： Generalized Statistics and Solar Neutrinos

摘要： 广义的Tsallis统计产生了一个适用于描述太阳内部等离子体的分布函数，该等离子体被视为恒星多态体，其尾部相对于麦克斯韦-玻尔兹曼分布被削弱，并且在能量大于约$20 \, k_{_B} T$时减少到零。 Tsallis统计理论上可以支持Clayton及其合作者过去提出的分布，该分布也显示出被削弱的尾部，用于解释太阳中微子计数率。 显示英文摘要

摘要： The generalized Tsallis statistics produces a distribution function appropriate to describe the interior solar plasma, thought as a stellar polytrope, showing a tail depleted respect to the Maxwell-Boltzmann distribution and reduces to zero at energies greater than about $20 \, k_{_B} T$. The Tsallis statistics can theoretically support the distribution suggested in the past by Clayton and collaborators, which shows also a depleted tail, to explain the solar neutrino counting rate.