Bardeen-Dirac stars in Anti-de Sitter spacetime

被引:0
作者
Zhang, Xiao-Yu [1 ,2 ,3 ]
Zhao, Li [1 ,2 ,3 ]
Wang, Yong-Qiang [1 ,2 ,3 ]
机构
[1] Lanzhou Univ, Lanzhou Ctr Theoret Phys, Sch Phys Sci & Technol, Key Lab Theoret Phys Gansu Prov, Lanzhou 730000, Peoples R China
[2] Lanzhou Univ, Inst Theoret Phys, Lanzhou 730000, Peoples R China
[3] Lanzhou Univ, Res Ctr Gravitat, Lanzhou 730000, Peoples R China
基金
中国国家自然科学基金;
关键词
gravity; GR black holes; stars; REGULAR BLACK-HOLES; GENERAL-RELATIVITY; BOSON STARS;
D O I
10.1088/1475-7516/2025/01/117
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we construct a static spherical symmetric Bardeen-Dirac stars (BDSs) in the four-dimensional Anti-de Sitter (AdS) spacetime, which consists of the electromagnetic field and Dirac field coupled to gravity. We investigate the ADM mass, No ether charge and light rings of BDSs in AdS spacetime. In asymptotically Minkowski spacetime, the maximum frequency of BDSs is one. However, we observe that the maximum frequency of BDSs increases as the cosmological constant decreases in AdS spacetime. Additionally, BDSs can exhibit extreme behavior at low frequencies, refer to as Frozen Bardeen-Dirac stars (FBDSs) in AdS spacetime. FBDSs have a critical event horizon, where the metric function g tt is very close to zero. The matter is entirely encapsulated by this critical horizon, highly concentrated within it. When the magnetic charge is fixed, the FBDSs gradually disappear as the cosmological constant decreases.
引用
收藏
页数:19
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