collaborators

9 papers

astro-ph.HE2026

The Environmental Effects on Inspiraling Binary Black Hole Systems in the Centers of the LMC and M31

Meng Xu, Zhijin Li, Xiao Guo +1

Binary black hole (BBH) systems residing in the centers of galaxies evolve within complex astrophysical environments. These environments, comprising dark matter (DM) halos and bary…

gr-qc2026

Stimulated Emission from Boson Clouds

Yu An, Xian-Hui Ge, Yun-Gui Gong +1

Gravitational-waves from astrophysical sources are characterized by their extreme faintness, which remains a primary obstacle for both current and next generation detectors. While…

gr-qc2026

Detecting gravitational wave background with equivalent configurations in the network of space based optical lattice clocks

Mingzhi Lou, Hong Su, Tao Yang +1

This paper studies the use of optical lattice clock (OLC) detector networks for detecting the stochastic gravitational-wave background (SGWB). Starting from the cross-correlation f…

hep-ph2026

Chiral Gravitational Wave Background from Audible Axion via Nieh-Yan Term

Baoyu Xu, Keyi Ding, Hong Su +2

Axions and axion-like particles can be probed through gravitational waves indirectly, often referred to as "audible axions". The usual concept of audible axion relies on the coupli…

gr-qc2026

Detecting Chiral Gravitational Wave Background with a Dipole Pulsar Timing Array

Baoyu Xu, Hanyu Jiang, Rong-Gen Cai +2

The pulsar timing array (PTA) is a powerful technique for detecting nanohertz gravitational wave backgrounds (GWBs). However, conventional PTAs lack sensitivity to parity violation…

gr-qc2025

Circularly Polarized Gravitational Wave Background Search with a Network of Space-borne Triangular Detectors

Ju Chen, Chang Liu, Yun-Long Zhang

Circularly polarized gravitational wave backgrounds are predicted in many well-motivated models of inflation and phase transitions involving spontaneous parity violation. In this w…