紧致的四维欧几里得空间嵌入宇宙

Y. Kurihara
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引用次数: 0

摘要

考虑一个紧致的四维流形,其度量张量具有正行列式(称为“欧几里得球”)。欧几里得球可以浸入闵可夫斯基空间(具有负行列式),并且可以通过宇宙的历史稳定存在。由于欧几里得球在其三维表面上与史瓦西黑洞具有相同的解,因此渐近观察者无法区分它们。如果前宇宙全部能量的很大一部分被封装在欧几里得球中,它们的行为就像当前宇宙中的暗物质。欧几里得球在宇宙膨胀的末期就已经存在了,在这个模型中,它们的质量很重,它们可能是超大质量黑洞的种子,这是早期宇宙中星系形成的必要条件。早期宇宙的伽马射线暴也可能是欧几里得球的信号。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Compact four–dimensional euclidean space embedded in the universe
A compact four-dimensional manifold whose metric tensor has a positive determinant (named the "Euclid ball") is considered. The Euclid ball can be immersed in the Minkovskian space (which has the negative determinant) and can exist stably through the history of the universe. Since the Euclid ball has the same solution as the Schwarzschild black hole on its three-dimensional surface, an asymptotic observer can not distinguish them. If large fraction of whole energy of the pre-universe was encapsulated in Euclid balls, they behave as the dark matter in the current universe. Euclid balls already existed at the end of the cosmological inflation, and can have a heavy mass in this model, they can be a seed of supper-massive black-holes, which are necessary to initiate a forming of galaxies in the early universe. The $\gamma$-ray burst at early universe is also a possible signal of the Euclidean ball.
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