We prove that for there does not exist a continuous map $\partial CV(F_k)\to\mathbb PCurr(F_k)Out(F_k)Out(F_k)\partial CV(F_k)$ is the “length-function” boundary of Culler-Vogtmann’s Outer space , and is the space of projectivized geodesic currents for . We also prove that, if , for the action of on and for the diagonal action of on the product space $\partial CV(F_k)\times \mathbb PCurr(F_k)Out(F_k)k\ge 3Out(F_k)CV(F_k)\mathbb PCurr(F_k)$ (such as the Patterson-Sullivan embedding) produces a new compactification of Outer space, different from the usual “length-function” compactification .

生成讲解博客的中文版本

生成AI智能校验的中文版本