暗星:超大质量和超质量暗宏观天体

Vladimir S. Netchitailo
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摘要

R. Genzel和A. Ghez因发现人马座A*是一个超大质量致密天体而被授予2020年诺贝尔物理学奖,而超大质量黑洞(SBH)是唯一被接受的解释。2013年,我们对超大质量致密天体提出了一种截然不同的解释:“世界上的宏观天体有由所讨论的DM粒子组成的核心。其他粒子,包括DM和重子物质,在核心“[1]”周围形成壳层。根据发展的超球世界-宇宙模型(WUM),世界由暗物质(约占总物质的92.8%)和普通物质(约占7.2%)组成。这意味着暗物质(DM)应该在任何宇宙模型中扮演主要角色。在WUM中就是这样,普通物质是暗物质粒子(dmp)自我湮灭的副产品。本文讨论了暗物质框架中的暗星、超大质量和超大质量暗天体。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dark Stars: Supermassive and Ultramassive Dark Macroobjects
R. Genzel and A. Ghez were awarded the 2020 Nobel Prize in Physics for their discovery that Sgr A* is a supermassive compact object, for which Supermassive Black Hole (SBH) was the only accepted explanation. In 2013, we proposed a principally different explanation of supermassive compact objects: “Macroobjects of the World have cores made up of the discussed DM particles. Other particles, including DM and baryonic matter, form shells surrounding the cores” [1]. According to the developed Hypersphere World-Universe Model (WUM), the World consists of Dark Matter (about 92.8% of the total Matter) and Ordinary matter (about 7.2%). It means that Dark Matter (DM) should play the main role in any Cosmological model. It is the case in WUM, and Ordinary matter is a byproduct of Dark Matter Particles (DMPs) self-annihilation. In present paper, we discuss Dark Stars, Supermassive and Ultramassive Dark Macroobjects in frames of WUM.
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