原初黑洞
Primordial black holes
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中文总结 AI 辅助
本综述介绍原初黑洞的形成模型，阐述利用天文与天体物理观测检验这些模型的方法，重点讨论闭合畴壁坍缩、宇宙额外空间维度效应形成原初黑洞及其星团的过程。
中文摘要 AI 辅助
原初黑洞由雅科夫·鲍里索维奇·泽尔多维奇和伊戈尔·德米特里耶维奇·诺维科夫于1966年首次提出其在早期宇宙中形成的假设（该开创性文章的文本收录于本综述的附录II），近年来受到越来越多关注。现代电磁全波段天文数据、引力波与宇宙中微子观测，揭示了一系列可能与恒星前宇宙时期形成的原初黑洞相关的独特天体物理现象。本综述阐述了多种原初黑洞形成模型，以及利用天文与天体物理观测检验这些模型的方法，尤其详细讨论了闭合畴壁坍缩、宇宙额外空间维度相关效应所导致的原初黑洞及其星团的形成过程。
英文摘要
Primordial black holes, whose formation in the early Universe was first hypothesized by Ya.B.~Zel'dovich and I.D.~Novikov in 1966 (the text of this pioneering article is provided in Appendix II to this review), have attracted increasing attention in recent years. Modern astronomical data across the electromagnetic spectrum, together with observations of gravitational waves and cosmic neutrinos, have revealed a number of unique astrophysical phenomena that may be related to primordial black holes formed in the pre-stellar cosmological epoch. This review describes various models of primordial black hole formation, as well as methods for testing these models with astronomical and astrophysical observations. In particular, we discuss in detail the formation of primordial black holes and their clusters through the collapse of closed domain walls and through effects associated with extra spatial dimensions of the Universe.
发表机构
- Institute for Nuclear Research of the Russian Academy of Sciences（俄罗斯科学院核物理研究所）
- National Research Nuclear University MEPhI（国立核研究大学莫斯科工程物理学院）
- Sternberg Astronomical Institute, Lomonosov Moscow State University（莫斯科罗蒙诺索夫国立大学斯捷尔伯格天文学研究所）
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