早期宇宙中的原星形成
Naoki Yoshida1, Kazuyuki Omukai, Lars Hernquist
1Department of Physics, Nagoya University, Furocho, Chikusa, Nagoya, Aichi 464-8602, Japan. nyoshida@a.phys.nagoya-u.ac.jp
概括
科学家模拟了第一颗恒星的形成. 大爆炸密度波动可以播下一个微小的原星,这是大质量原始恒星的前体.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 恒星进化 恒星进化
背景情况:
- 早期宇宙中第一个恒星 (人群III恒星) 的形成和性质尚不清楚.
- 理论上,宇宙结构的增长是通过引力不稳定性层次发生的.
- 观测证据表明,早期宇宙中存在大质量原始恒星.
研究的目的:
- 通过初始计算机模拟来研究第一个恒星的形成机制.
- 在一个膨胀的宇宙中,模拟原始气体中的原子和分子过程.
主要方法:
- 开发了一个初始的计算机模拟.
- 通过跟踪原子和分子过程来模拟原始恒星的形成.
- 纳入了一个膨胀宇宙模型.
主要成果:
- 模拟表明,从大爆炸开始的原始密度波动可以启动恒星形成.
- 一个微小的原星,大约占太阳质量的1%,可以从这些波动中形成.
- 这颗原恒星作为后续发展大质量原始恒星的种子.
结论:
- 原始密度波动是启动第一个恒星形成的可行机制.
- 该模拟为了解早期宇宙中大质量恒星的起源提供了一条途径.
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