Schwarzschild-Levi-Civita black hole

IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics Letters B Pub Date : 2025-02-01 DOI:10.1016/j.physletb.2024.139234
S. Habib Mazharimousavi
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Abstract

Inspired by the geometry of the Ernst black hole which interpolates the static spherically symmetric Schwarzschild black hole and the static axially symmetric magnetic Melvin spacetime, in this paper, we aim to present a solution to Einstein's field equation in vacuum to interpolate the Schwarzschild black hole and the Levi-Civita spacetime. Hence, we shall call the solution the Schwarzschild-Levi-Civita black hole. Effectively the solution is a two-parameter non-asymptotically flat black hole that is static, axially symmetric, and singular in its axis of symmetry.
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史瓦西-列维-奇维塔黑洞
受恩斯特黑洞插入静态球对称史瓦西黑洞和静态轴对称磁梅尔文时空的几何启发,本文旨在提出真空中爱因斯坦场方程的解,以插入史瓦西黑洞和列维-奇维塔时空。因此,我们将这个解称为史瓦西-列维-奇维塔黑洞。有效的解决方案是一个静态的、轴对称的、对称轴奇异的双参数非渐近平坦黑洞。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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