强大的准星黑洞的回弹：来自强劲类星体的证据

Marco Chiaberge; Takahiro Morishita; Matteo Boschini; Stefano Bianchi; Alessandro Capetti; Gianluca Castignani; Davide Gerosa; Masahiro Konishi; Shuhei Koyama; Kosuke Kushibiki; Erini Lambrides; Eileen T. Meyer; Kentaro Motohara; Massimo Stiavelli; Hidenori Takahashi; Grant R. Tremblay; Colin Norman

强大的准星黑洞的回弹：来自强劲类星体的证据

星系天体物理 2025-02-24 v2 广义相对论与量子宇宙学

作者: Marco Chiaberge , Takahiro Morishita , Matteo Boschini , Stefano Bianchi , Alessandro Capetti , Gianluca Castignani , Davide Gerosa , Masahiro Konishi , Shuhei Koyama , Kosuke Kushibiki , Erini Lambrides , Eileen T. Meyer , Kentaro Motohara , Massimo Stiavelli , Hidenori Takahashi , Grant R. Tremblay , Colin Norman

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摘要

超大质量黑洞(SMBH)通过吸积物和 mergers 增长。SMBH mergers 长期面临最终太阳系问题，即 SMBH 二元在引力波能量损失显著之前可能停滞，导致双黑洞未被合并。直接的已合并 SMBH 证据仍然稀少。理论预测，随着黑洞 mergers 后可发生 GW recoiling 黑洞。本文提供新的且具有结论性的光谱证据，表明 3C 186 这一空间偏移类星体的吸积盘和宽线区均以相同速度向蓝端偏移，线视速度为(-1310 ± 21) km/s。这最佳解释为 GW recoil super-kick 场景。这一确认了撞击过程，意味着最终太阳系问题在自然界中得到解决，表明即便是最质量的黑洞也能被合并。

关键词

超大质量黑洞类星体引力波回弹 3C 186 Rashba 效应

引用

@article{arxiv.2501.18730,
  title  = {A recoiling supermassive black hole in a powerful quasar},
  author = {Marco Chiaberge and Takahiro Morishita and Matteo Boschini and Stefano Bianchi and Alessandro Capetti and Gianluca Castignani and Davide Gerosa and Masahiro Konishi and Shuhei Koyama and Kosuke Kushibiki and Erini Lambrides and Eileen T. Meyer and Kentaro Motohara and Massimo Stiavelli and Hidenori Takahashi and Grant R. Tremblay and Colin Norman},
  journal= {arXiv preprint arXiv:2501.18730},
  year   = {2025}
}

备注

32 pages, 10 figures, submitted

强大的准星黑洞的回弹：来自强劲类星体的证据

摘要

关键词

引用

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