Supported by the National Natural Science Foundation of China(NNSFC)(11805166,11925503,12175076);the financial support from Fundacao de Amparo a Pesquisa do Estado de Sao Paulo(FAPESP);Fundacao de Amparo a Pesquisa do Estado do Rio de Janeiro(FAPERJ);Conselho Nacional de Desenvolvimento Científico e Tecnológico(CNPq);Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior(CAPES);the project Institutos Nacionais de Ciencias e Tecnologia-Fisica Nuclear e Aplicacoes(INCT/FNA)Proc.No.464898/2014-5;supported by the Center for Scientific Computing(NCC/Grid UNESP)of the Sao Paulo State University(UNESP)。
In this study,we investigate the quasinormal mode and late-time tail of charged massless scalar perturbations of a black hole in generalized Rastall gravity.The black hole metric in question is spherically symmetric,a...
Supported by Natural Science Foundation of China(11605152,11675139,51802247)。
We study quasinormal modes(QNMs)of charged black holes in the Einstein-Maxwell-Weyl(EMW)gravity by adopting the test scalar field perturbation.We find that the imaginary part of QNM frequencies is consistently negativ...
NSFC(Grant No.11505119,11005016,11875196 and 11375121)。
It has been shown that the quasinormal modes of perturebated fields can be used to investigate the validity of strong cosmic censorship(SCC).Relevant issues for Reissner-Nordstrom-de Sitter(RN-dS)black holes and Born-...
supported by National Nature Science Foundation of China (Grant No. 11771409);Wu Wen-Tsun Key Laboratory of Mathematics of Chinese Academy of Sciences
Let σ={σi | i ∈ I} be some partition of the set of all primes P. A set H of subgroups of G is said to be a complete Hall σ-set of G if every member ≠ 1 of H is a Hall σi-subgroup of G, for some i ∈ I, and H con...
Supported by the National Nature Science Foundation of Education Department of Shannxi Province under Grant No.15JK1077;the Doctorial Scientific Research Starting Fund of Shannxi University of Science and Technology under Grant No.BJ12-02
The quasinormal modes of the Schwarzschild black hole surrounded by the quintessence in Rastall gravity are studied using the sixth-order Wentzel-Kramers-Brillouin approximative approach. The effect of the Rastall par...
Based on the well known fact that the quasinormal frequencies are the poles of the frequency domain Green’s function we describe a method that allows us to calculate exactly the quasinormal frequencies of the Klein-G...
Supported by the National Natural Science Foundation of China(Grant Nos.11501075,11271059);the Natural Science Foundation of Liaoning Education Department(Grant No.L2015084);the Natural Science Foundation of Guangxi Education Department(Grant No.KY2015LX518)
In this paper, we study some properties of dual Toeplitz operators on the orthog- onal complement of Bergman space of the unit ball. We first completely characterize the boundedness and compactness of dual Toeplitz op...
Supported by King Saud University, Deanship of Scientific Research, College of Science Research Center
Dual Toeplitz operators on the Hardy space of the unit circle are anti-unitarily equivalent to Toeplitz operators. In higher dimensions, for instance on the unit sphere, dual Toeplitz operators might behave quite diff...
The Heun functions have wide application in modern physics and are expected to succeed the hypergeometrical functions in the physical problems of the 21st century. The numerical work with those functions, however, is ...
Supported by the National Natural Science Foundation of China (Grant No. 10773002)
Using the spin networks and the asymptotic quasinormal mode frequencies of black holes given by loop quantum gravity,the minimum horizon area gap is obtained.Then the quantum area spectrum of black holes is derived an...