标题： 中微子触发和中子星到奇异星的转化 显示英文标题

标题： Neutrino sparking and the neutron to strange stars conversion

摘要： 我们通过高能中微子相互作用（引发）来研究中子星内部奇异团的产生。 要求中子星在其整个生命周期内保持为中子星，我们得到了最终态中奇异团的概率上限，并将其与现有的实验室限制进行比较。 结果表明，对于产生夸克-胶子等离子体所需的最小中心质量能量的实际值，这种机制不太可能驱动中子$\to$奇异星的转换，这是奇异团形成的一个必要前提条件。 显示英文摘要

摘要： We address the production of strangelets inside neutron stars by means of high-energy neutrino interactions (sparking). Requiring that neutron stars remain as such along their lifetimes, we obtain a bound on the probability of a strangelet in the final state and compare it with existing laboratory limits. It turns out that this mechanism is not likely to drive a neutron $\to$ strange stars conversion for realistic values of the minimum center-mass-energy necessary to produce the quark-gluon plasma, a necessary precondition for the formation of the strangelet.