膨胀宇宙中的量子黑洞

IF 0.6 4区物理与天体物理 Q4 MECHANICS

Doklady Physics Pub Date : 2024-02-15 DOI:10.1134/S1028335823070042

V. P. Neznamov, I. I. Safronov, V. E. Shemarulin

引用次数: 0

摘要

摘要在膨胀的宇宙中，我们考虑了具有修正的施瓦兹柴尔德几何和赖斯纳-诺德斯特伦几何的量子黑洞的演化。在宇宙学时间的特定时刻，所有量子黑洞都会失去事件视界，并转化为质量为 M 的引力物体。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Quantum Black Holes in the Expanding Universe

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Quantum Black Holes in the Expanding Universe

In the expanding Universe, the evolution of quantum black holes with modified Schwarzschild and Reissner–Nordström geometries is considered. All quantum black holes at definite moments of the cosmological time lose event horizons and are transformed to gravitating objects with masses M.

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来源期刊

Doklady Physics 物理-力学

CiteScore

1.40

自引率

12.50%

发文量

审稿时长

4-8 weeks

期刊介绍： Doklady Physics is a journal that publishes new research in physics of great significance. Initially the journal was a forum of the Russian Academy of Science and published only best contributions from Russia in the form of short articles. Now the journal welcomes submissions from any country in the English or Russian language. Every manuscript must be recommended by Russian or foreign members of the Russian Academy of Sciences.