collaborators

5 papers

astro-ph.HE2026

Relativistic Thermal Emission from Accretion Disks in Kerr-MOG Spacetimes

Cheng Liu, Xu-fan Hu, Yosuke Mizuno +1

In Scalar-Tensor-Vector Gravity (STVG, also known as MOG), a massive vector field generates a repulsive fifth force that endows rotating black holes with a gravitational ch…

astro-ph.HE2026

Signature of iron line profile from a Kerr-like wormhole

Cheng Liu, Hoongwah Siew, Hong-Xuan Jiang +2

Broad, skewed iron K emission lines in the X-ray spectra of accreting black holes encode key information about the spacetime geometry of the innermost disk. While the Kerr metr…

gr-qc2024

Two distinct types of echoes in compact objects

Shui-Fa Shen, Kai Lin, Tao Zhu +3

In the black hole perturbation theory framework, two different physical pictures for echoes in compact objects have been proposed. The first mechanism interprets echoes as repeated…

gr-qc2024

Observational test of spacetimes with the S2 star in the Milky Way galactic center

Jian-Ming Yan, Tao Zhu, Mustapha Azreg-Aïnou +2

A novel class of vacuum metrics expressible in analytical form was recently found for pure gravity, based on a groundwork put forth by Buchdahl in 1962. These Buchda…

astro-ph.HE2024

The Heavier the Faster: A Sub-population of Heavy, Rapidly Spinning and Quickly Evolving Binary Black Holes

Wei-Hua Guo, Yin-Jie Li, Yuan-Zhu Wang +4

The spins of binary black holes (BBHs) measured from gravitational waves carry notable information of the formation pathways. Here we propose a quantity "dimensionless net spin" ($…