论文标题
人口III星的质量间隙紧凑物体和黑洞二进制的形成
Formation of mass gap compact object and black hole binary from Population III stars
论文作者
论文摘要
当形成MGCOS（质量间隙紧凑的物体2--5 $ \，M _ {\ odot} $）时，我们对具有Maxwellian Kick速度分布的种群III二元星的种群合成模拟。我们发现，对于$σ_ {\ rm k} = 0 $ - $ 500 $ km/s的八个踢速度分散模型，黑洞的平均质量（bh）-mgco二进制质量为$ \ sim（30 \，m_ \ odot，\ odot，\，\，2.6 \，2.6 \，m_ \ odot）$。在模拟的数值数据中，我们发现BH-MGCO二进制的存在具有质量$（22.9 \，m_ \ odot，\，\，2.5 \，m_ \ odot）$，看起来像GW190814。
We performed population synthesis simulations of Population III binary stars with Maxwellian kick velocity distribution when MGCOs (Mass Gap Compact Objects with mass 2--5$\,M_{\odot}$) are formed. We found that for eight kick velocity dispersion models of $σ_{\rm k}=0$--$500$ km/s, the mean mass of black hole (BH)-MGCO binary is $\sim (30 \,M_\odot,\,2.6 \,M_\odot)$. In numerical data of our simulations, we found the existence of BH-MGCO binary with mass $(22.9 \,M_\odot,\,2.5 \,M_\odot)$ which looks like GW190814.
