collaborators

8 papers

astro-ph.HE2026

Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals

Tian-Xiao Wang, Yan Wang, Alejandro Torres-Orjuela +4

Extremely large mass-ratio inspirals (XMRIs), consisting of a brown dwarf orbiting a supermassive black hole, emit long-lived and nearly monochromatic gravitational waves in the mi…

gr-qc2025

Constraining modified theories of gravity through the detection of one extremely large mass-ratio inspiral

Hui-Min Fan, Alejandro Torres-Orjuela, Verónica Vázquez-Aceves +2

Extremely large mass-ratio inspirals (XMRIs), formed by brown dwarfs inspiraling into a massive black hole, emit gravitational waves (GWs) that fall within the detection band of fu…

gr-qc2025

Constraining the EdGB Theory with Extreme Mass-Ratio Inspirals

Jing Tan, Jian-dong Zhang, Hui-Min Fan +1

The Einstein-dilaton-Gauss-Bonnet (EdGB) theory is a modified theory of gravity which include a scalar field to couple with the higher order curvature terms. It has already been co…

gr-qc2025

Observational properties of black hole in quantum fluctuation modified gravity

Jiajun Yin, Tong-Yu He, Ming Liu +4

This study investigates the properties of the thin accretion disk around a black hole in quantum fluctuation modified gravity (QFMGBH) using the Novikov-Thorne model. We restrict t…

gr-qc2025

GWSpace: a multi-mission science data simulator for space-based gravitational wave detection

En-Kun Li, Han Wang, Hong-Yu Chen +11

Space-based gravitational wave detectors such as TianQin, LISA, and TaiJi have the potential to outperform themselves through joint observation. To achieve this, it is desirable to…

astro-ph.HE2025

Probing the Extreme-Mass-Ratio Inspirals Population Constraints with TianQin

Hui-Min Fan, Xiang-Yu Lyu, Jian-dong Zhang +3

Extreme-mass-ratio inspirals (EMRIs), consisting of a massive black hole and a stellar compact object, are one of the most important sources for space-borne gravitational wave dete…