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超大质量黑洞的直接形成是通过星系合并的多层次气体流入而形成的
L Mayer1, S Kazantzidis, A Escala
1Institute for Theoretical Physics, University of Zürich, 190 Winterthurestrasse, Zürich 8057, Switzerland. lmayer@physik.unizh.ch
Nature
|August 27, 2010
概括
大规模原星系的合并可以自然形成超大质量黑洞. 这些合并创造了直接气体崩的条件,绕过了抑制恒星形成的需要,使黑洞快速生长.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
- 黑洞形成的过程
背景情况:
- 数十亿太阳质量的超大质量黑洞 (SBHs) 存在于宇宙早期,大爆炸后不到十亿年.
- 以前的模型涉及原始恒星崩或孤立原星系的直接崩,由于低效的气体积聚或严格的环境要求,难以解释这些早期SBHs的快速形成和增长.
研究的目的:
- 为了研究超大质量黑洞快速形成的新机制.
- 为了确定原银河的合并是否可以自然地促进直接崩成为巨大的黑洞,而不需要抑制冷却或恒星形成.
主要方法:
- 数字模拟合并的大质量原星系的数字模拟.
- 分析气体动力学,积累速度和聚合驱动的核气体盘中的引力崩.
主要成果:
- 原星系的合并自然会产生不稳定的,巨大的核气盘.
- 这些磁盘在10万年内有效地将大量气体 (超过108太阳质量) 输送到亚帕塞克尺度.
- 这种快速的气体度触发了引力崩,形成了一个巨大的黑洞种子.
结论:
- 合并驱动的气体流入为直接崩提供了一个可行的途径,在没有异国情调的情况下形成SBH种子.
- 模拟的机制解释了在早期宇宙中观察到的SBHs的快速出现.
- 随后这些种子上的积累可以在108年内导致数十亿太阳质量黑洞.
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