Supported by FAPESP(2012/08934-0);National Natural Science Foundation of China(11205254,11178018,11375279,11605015);the Natural Science Foundation Project of CQ CSTC(2011BB0052);the Fundamental Research Funds for the Central Universities(106112016CDJXY300002,106112017CDJXFLX0014,CDJRC10300003)
In this paper, we describe quasinormal modes(QNMs) for gravitational perturbations of Einstein-GaussBonnet black holes(BHs) in higher dimensional spacetimes, and derive the corresponding parameters of such black h...
Supported by National Natural Science Foundation of China(11605015,11375279,11205254,11647307);the Fundamental Research Funds for the Central Universities(106112017CDJXY300003,106112017CDJXFLX0014)
Extremely powerful astrophysical electromagnetic(EM) systems could be possible sources of highfrequency gravitational waves(HFGWs). Here, based on properties of magnetars and gamma-ray bursts(GRBs), we address ...
supported by the National Natural Science Foundation of China(Grant Nos.11205254,11178018,11375279,and 11605015);the Fundamental Research Funds for the Central Universities,China(Grant Nos.106112016CDJXY300002 and CDJRC10300003);the Chinese State Scholarship Fund,FAPESP(Grant No.2012/08934-0);the Natural Science Foundation Project of CQ CSTC(Grant No.2011BB0052)
In this paper, we study the gravitational quasi-normal modes(QNMs) for a static R^2 black hole(BH) in Anti-de Sitter(AdS) spacetime. The corresponding master equation of odd parity is derived and the QNMs are ev...
Project supported by the National Natural Science Foundation of China(Grant Nos.11075224 and 11375279);the Foundation of China Academy of Engineering Physics(Grant Nos.2008 T0401 and T0402)
Various cosmology models, brane oscillation scenarios, interaction of interstellar plasma with intense electromagnetic radiation, and even high-energy physics experiments (e.g., Large Hadron Collider (LHC)) all pr...