Stability of Cauchy horizon in a charged de-Sitter spacetime with dark matter

被引:3
|
作者
Nan, Xue-Ying [3 ]
Tan, Jia [2 ]
Jiang, Jie [1 ]
机构
[1] Beijing Normal Univ, Coll Educ Future, Zhuhai 519087, Peoples R China
[2] Suzhou Univ Sci & Technol, Sch Phys Sci & Technol, Jiangsu Key Lab Micro & Nano Heat Fluid Flow Techn, Suzhou 215009, Peoples R China
[3] Nankai Univ, Coll Elect Informat & Opt Engn, Dept Microelect Engn, Tianjin 300350, Peoples R China
来源
EUROPEAN PHYSICAL JOURNAL C | 2023年 / 83卷 / 05期
基金
中国国家自然科学基金;
关键词
QUASI-NORMAL MODES; BLACK-HOLES; COSMIC CENSORSHIP; VECTOR FIELD; SITTER;
D O I
10.1140/epjc/s10052-023-11627-3
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The violation of strong cosmic censorship (SCC) in RNdS black holes by a minimally coupled neutral massless scalar field has recently been discovered. This paper investigates the stability of the Cauchy horizon of a spherically charged de-Sitter black hole surrounded by dark matter under perturbations from a massless scalar field. Our results show that SCC can also be destroyed in the nearly extremal region, regardless of the presence of dark matter. However, the existence of dark matter can mitigate the extent of SCC violation, particularly when the cosmological constant and dark matter energy density are both small. Notably, the violation region of SCC as a function of the dark matter state parameter does not exhibit a simple monotonic decrease, suggesting that the influence of dark matter on SCC is not straightforward and may be complex.
引用
收藏
页数:8
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