collaborators

5 papers

gr-qc2026

Probing near-zone magnetic fields with extreme mass-ratio inspirals

Jin-Lu Hu, Xin-Dong Du, Peng-Cheng Li +1

We investigate whether weak near-zone magnetic fields can leave observable imprints on extreme-mass-ratio inspiral (EMRI) waveforms. The central massive black hole is modeled by th…

gr-qc2026

Quasinormal mode/grey-body factor correspondence for Kerr black holes

Zun-Xian Huang, Peng-Cheng Li

We revisit the quasinormal-mode/greybody factor correspondence for Kerr black holes in the eikonal limit and develop a systematic WKB-based formulation by recasting the radial Teuk…

gr-qc2025

Constraint on massive vector field with extreme-mass-ratio inspirals around a slowly rotating black hole

Tieguang Zi, Peng-Cheng Li, Bao-Min Gu +1

We study the influence of a massive vector (Proca) field on the energy fluxes from extreme-mass-ratio inspirals (EMRIs) around a slowly rotating Kerr black hole. The secondary comp…

gr-qc2025

Detection of a Higher Harmonic Quasi-normal Mode in the Ringdown Signal of GW231123

Hai-Tian Wang, Shao-Peng Tang, Peng-Cheng Li +1

The ringdown phase of a gravitational wave signal from a binary black hole merger offers a unique laboratory for testing general relativity in the strong-field regime and probing t…

gr-qc2025

Stable massless scalar polarization of f(R) gravity

Xin-Dong Du, Peng-Cheng Li

Polarization is a prominent feature of gravitational wave observations and can be used to distinguish between different modified gravity theories. Compared to General Relativity, f…