GWTC-4.0：合并致密二进制的天体物理属性
高能天体物理现象
2025-09-19 v2 广义相对论与量子宇宙学
摘要
我们详细描述了使用来自累计引力波瞬态目录 4.0（包含 158 个合祸事件）的致密天体合并的天体物理属性，该目录包括三种类型的二进制合祸：二进制中子星、中子星-黑洞二进制和二进制黑洞合祸。我们解决了黑洞质量分布中多个过-不足密度：在主质量为 和 处均存在特征，且可能在约 处存在第三个特征。这些是来自否则呈幂律样连续体的偏离，上方趋于变陡。主质量接近 的二进制黑洞更可能拥有较轻的次级质量，其质量比分布在 处峰值，这可能是稳定质量传递 During binary evolution 的特征。黑洞自旋被推断为非极限值，其中 90% 的黑洞具有 ，且倾向于与二进制轨道对齐，这表明许多合并二进制在孤立条件下形成。然而，我们发现显著比例（0.24-0.42）的二进制具有负的有效灵流自旋，这暗示许多可能是在无气体环境中形成。我们发现有效灵流自旋与质量比之间存在相关性，尽管尚不清楚这是由分布模式的变化还是宽度决定的。（已节选）
引用
@article{arxiv.2508.18083,
title = {GWTC-4.0: Population Properties of Merging Compact Binaries},
author = {The LIGO Scientific Collaboration and the Virgo Collaboration and the KAGRA Collaboration and A. G. Abac and I. Abouelfettouh and F. Acernese and K. Ackley and C. Adamcewicz and S. Adhicary and D. Adhikari and N. Adhikari and R. X. Adhikari and V. K. Adkins and S. Afroz and D. Agarwal and M. Agathos and M. Aghaei Abchouyeh and O. D. Aguiar and S. Ahmadzadeh and L. Aiello and A. Ain and P. Ajith and T. Akutsu and S. Albanesi and R. A. Alfaidi and A. Al-Jodah and C. Alléné and A. Allocca and S. Al-Shammari and P. A. Altin and S. Alvarez-Lopez and O. Amarasinghe and A. Amato and C. Amra and A. Ananyeva and S. B. Anderson and W. G. Anderson and M. Andia and M. Ando and T. Andrade and M. Andrés-Carcasona and T. Andrić and J. Anglin and S. Ansoldi and J. M. Antelis and S. Antier and M. Aoumi and E. Z. Appavuravther and S. Appert and S. K. Apple and K. Arai and A. Araya and M. C. Araya and M. Arca Sedda and J. S. Areeda and L. Argianas and N. Aritomi and F. Armato and S. 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Xu and Y. Xu and N. Yadav and H. Yamamoto and K. Yamamoto and T. S. Yamamoto and T. Yamamoto and S. Yamamura and R. Yamazaki and T. Yan and F. W. Yang and F. Yang and K. Z. Yang and Y. Yang and Z. Yarbrough and H. Yasui and S. -W. Yeh and A. B. Yelikar and X. Yin and J. Yokoyama and T. Yokozawa and J. Yoo and H. Yu and S. Yuan and H. Yuzurihara and A. Zadrożny and M. Zanolin and M. Zeeshan and T. Zelenova and J. -P. Zendri and M. Zeoli and M. Zerrad and M. Zevin and A. C. Zhang and L. Zhang and R. Zhang and T. Zhang and Y. Zhang and C. Zhao and Yue Zhao and Yuhang Zhao and Y. Zheng and H. Zhong and R. Zhou and X. -J. Zhu and Z. -H. Zhu and A. B. Zimmerman and M. E. Zucker and J. Zweizig},
journal= {arXiv preprint arXiv:2508.18083},
year = {2025}
}
备注
As part of the Astrophysical Journal Letters Focus Issue on the Gravitational Wave Transient Catalog