MESA input and results for: A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up

MESA inlists, input files and associated data products for the paper "A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up". Version 15140 is used. BH-He stars binary evolution result data are included in ''result.zip'', and folders name match the initial parameters of system, e.g. BHs mass, He-rich stars mass, periods, accretion rates limit. The detailed evolution history is in file ''history.data'', where its initial parameters match the folder name. We evolve He-rich stars until the carbon depletion is reached in the center, we suggest the last line of ''history.data'' is the end of BH-He rich stars evolution course. BH-NS binary systems evolution sim based on these data with method described in the article.本数据集包含用于论文《作为多信使源的快速旋转黑洞-中子星双星并合形成路径 Ⅱ. 吸积致自转加速》的MESA输入列表文件、输入文件及关联数据产物，采用版本15140。黑洞-氦星双星演化结果数据存放于`result.zip`压缩包中，各文件夹名称与对应双星系统的初始参数一一对应，例如黑洞质量、富氦星质量、轨道周期、吸积率上限。详细演化历史存储于`history.data`文件中，该文件的初始参数与对应文件夹的名称完全匹配。本次演化将富氦星演化至中心碳耗尽状态，建议将`history.data`的最后一行作为黑洞-富氦星双星演化过程的终止节点。本数据集还包含基于上述数据、采用论文所述方法完成的黑洞-中子星（BH-NS）双星系统演化模拟结果。