Abstract
AbstractIn this work, we first calculate equations of motion for particles in the Kerr-Sen-de Sitter black hole spacetime. Then, in the eikonal regime, we analytically obtain the quasi-normal resonant modes of massless neutral scalar field perturbation and find its imaginary part to be characterized by the surface gravity of a near-extremal Kerr-Sen-de Sitter black hole with the Cauchy horizon approaching the event horizon. We further show that the Penrose strong cosmic censorship conjecture is thus respected in this spacetime with dilaton scalar field and axion pseudoscalar field.
Funder
National Natural Science Foundation of China
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Reference70 articles.
1. R. Penrose, Riv. Nuovo Cim. 1, 252 (1969)
2. D. Christodoulou, in 12th Marcel Grossmann Meeting on General Relativity (2008). arXiv:0805.3880 [gr-qc]
3. M. Simpson, R. Penrose, Int. J. Theor. Phys. 7, 183 (1973)
4. E. Poisson, W. Israel, Phys. Rev. D 41, 1796 (1990)
5. M. Dafermos, Commun. Pure Appl. Math. 58, 0445 (2005). arXiv:gr-qc/0307013
Cited by
1 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献