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20232026
most citedComplete quasinormal modes of Type-D black holes

7 citations · 19 across the 10 of their papers we have counts for

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gr-qc2026

Complete total-transmission modes of Kerr black holes

Changkai Chen, Xiaohua Zhang, Zhoujian Cao +2

We construct the complete spectrum of gravitational total-transmission modes (TTMs) of Kerr black holes and find four globally continuous families, , each with tw…

hep-th2026

Holographic subregion complexity in unbalanced Stückelberg holographic superconductors

Yu Shi, Chikun Ding, Yuebing Zhou +2

Within the subregion complexity-volume conjecture, we numerically compare holographic subregion complexity (HSC) and holographic entanglement entropy (HEE) for a strip in unbalance…

gr-qc2026

Images of Braneworld black holes with radiatively inefficient accretion flows

Chengjia Chen, Yin Hao, Zelin Zhang +2

Horizon-scale imaging acts as a transformative tool for probing spacetime geometry, enabling stringent tests of gravitational theories in the strong-field regime. The Casadio-Fabbr…

gr-qc2026

Efficient and stable computation of gravitational-wave fluxes from generic Kerr orbits via a unified Heun-function framework

Changkai Chen, Zhoujian Cao, Jiliang Jing

Modeling extreme-mass-ratio inspirals hinges on the accurate and efficient computation of gravitational-wave fluxes from generic Kerr orbits. Conventional frequency-domain techniqu…

gr-qc2026

Quasinormal modes and AdS/CFT correspondence of a rotating BTZ-like black hole in the Einstein-bumblebee gravity

Fangli Quan, Zhong-Wu Xia, Rui Ding +2

We obtain exact expressions for the quasinormal modes (QNMs) of the massive scalar, fermionic and vector perturbations around a rotating BTZ-like black hole in the Einstein-bumbleb…

gr-qc2026

Charged scalar and Dirac perturbations on a global monopole Reissner-Nordström-de Sitter black hole: quasinormal modes and strong cosmic censorship

Peiyang Li, Mengjie Wang, Jiliang Jing

We study perturbations of charged scalar and Dirac fields around Reissner-Nordström-de Sitter black holes with a global monopole. To this end, we first derive the equations of moti…