collaborators

7 papers

astro-ph.HE2026

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap

Tian Huang, Xizhen Lu, Guoliang Lü +8

Observations of binary black hole (BBH) mergers detected by LIGO -- such as GW170729, GW190620, GW190706, GW230107, GW230820, and GW230928 -- feature high effective spins and prima…

astro-ph.SR2026

Evolution of cataclysmic variables under different magnetic braking prescriptions

Bingyao Zhou, Chunhua Zhu, Guoliang Lü +3

Context. The evolution of cataclysmic variables (CVs) - interacting binaries where a low-mass donor transfers matter to a white dwarf via an accretion disk - is critically controll…

astro-ph.SR2025

Formation of the Dormant Black Holes with Luminous Companions from Binary or Triple Systems

Zhuowen Li, Xizhen Lu, Guoliang Lü +6

Recently, a class of dormant black hole binaries with luminous companions (dBH-LC) has been observed, such as BH1, BH2, and BH3. Unlike previously discovered X-ray BH binari…

astro-ph.HE2025

Hunting Hidden Axion Signals in Pulsar Dispersion Measurements with Machine Learning

Haihao Shi, Zhenyang Huang, Qiyu Yan +3

In axion models, interactions between axions and electromagnetic waves induce frequency-dependent time delays determined by the axion mass and decay constant. These small delays ar…

astro-ph.SR2025

The influence of rotation and metallicity on the explodability of massive stars

Renyu Luo, Chunhua Zhu, Guoliang Lü +4

During the late stages of massive stellar evolution, failed supernovae (FSN) may form through core-collapse processes. The traditional evaluation criterion 0.45, pri…

astro-ph.SR2025

The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars

Zhijun Wang, Guoliang Lü, Chunhua Zhu +3

Context: Intermediate-mass asymptotic giant branch (AGB) stars influence Galactic lithium evolution by ejecting surface material (including Li) via stellar winds. Internal gravity…