标题： 星系等离子体和太阳中微子的非广延统计学 显示英文标题

标题： Nonextensive statistics in stellar plasma and solar neutrinos

摘要： 非广延性和量子不确定性效应（与恒星核心组成的准粒子有关）对核反应率有强烈影响，并且当然会影响太阳中微子流。 这两种效应同时存在，是由于离子间的频繁碰撞所致。 太阳核心的弱非广延性特性得到证实。 中微子流的预测范围扩大了，太阳中微子问题也不那么严重了。 显示英文摘要

摘要： Nonextensive and quantum uncertainty effects (related to the quasiparticles composing the stellar core) have strong influence on the nuclear rates and, of course, affect solar neutrino fluxes. Both effects do coexist and are due to the frequent collisions among the ions. The weakly nonextensive nature of the solar core is confirmed. The range of predictions for the neutrino fluxes is enlarged and the solar neutrino problem becomes less dramatic.