Quasinormal modes of regular black holes with sub-Planckian curvature and Minkowskian core

被引:0
作者
Tang, Chen [1 ]
Ling, Yi [1 ,2 ,3 ]
Jiang, Qing-Quan [1 ]
Li, Guo-Ping [1 ]
机构
[1] China West Normal Univ, Sch Phys & Astron, Nanchong 637002, Peoples R China
[2] Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China
[3] Univ Chinese Acad Sci, Sch Phys, Beijing 100049, Peoples R China
来源
EUROPEAN PHYSICAL JOURNAL C | 2024年 / 84卷 / 12期
基金
北京市自然科学基金;
关键词
GENERAL-RELATIVITY;
D O I
10.1140/epjc/s10052-024-13699-1
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
We investigate the perturbation of the scalar field as well as the electromagnetic field over a sort of regular black holes which are characterized by the sub-Planckian curvature and the Minkowskian core. Specifically, we compute the quasinormal modes (QNMs) by employing the pseudo-spectral method. The outburst of overtones is manifestly observed in the QNMs of these regular black holes, which can be attributed to the deviation of the Schwarzschild black hole by quantum effects of gravity. Furthermore, the QNMs under the perturbation of electromagnetic field exhibit smaller real and imaginary parts than those under scalar field perturbation. By comparing the QNMs of the regular black hole featured by Minkowskian core with those of Bardeen black hole featured by de Sitter core, we find they may be an effective tool to distinguish these BHs.
引用
收藏
页数:15
相关论文
共 109 条
  • [1] Nollert H.-P., TOPICAL REVIEW: Quasinormal modes: the characteristic ‘sound’ of black holes and neutron stars, Class. Quantum Gravity, 16, pp. R159-R216, (1999)
  • [2] Kokkotas K.D., Schmidt B.G., Quasi-normal modes of stars and black holes, Living Rev. Relativ, 2, pp. 1-72, (1999)
  • [3] Berti E., Cardoso V., Starinets A.O., Quasinormal modes of black holes and black branes, Class. Quantum Gravity, 26, 16, (2009)
  • [4] Konoplya R., Zhidenko A., Quasinormal modes of black holes: from astrophysics to string theory, Rev. Mod. Phys, 83, 3, pp. 793-836, (2011)
  • [5] Echeverria F., Gravitational-wave measurements of the mass and angular momentum of a black hole, Phys. Rev. D, 40, 10, (1989)
  • [6] Flanagan E.E., Hughes S.A., Measuring gravitational waves from binary black hole coalescences. II. The waves’ information and its extraction, with and without templates, Phys. Rev. D, 57, 8, (1998)
  • [7] Yang H., Nichols D.A., Zhang F., Zimmerman A., Zhang Z., Chen Y., Quasinormal-mode spectrum of Kerr black holes and its geometric interpretation, Phys. Rev. D-Part. Fields Gravit. Cosmol, 86, 10, (2012)
  • [8] Horowitz G.T., Hubeny V.E., Quasinormal modes of ads black holes and the approach to thermal equilibrium, Phys. Rev. D, 62, 2, (2000)
  • [9] Konoplya R.A., Zhidenko A., Stability of multidimensional black: complete holesnumerical analysis, Nucl. Phys. B, 777, 1-2, pp. 182-202, (2007)
  • [10] Konoplya R.A., Zhidenko A., Instability of higher-dimensional charged black holes in the de sitter world, Phys. Rev. Lett, 103, 16, (2009)