collaborators

9 papers

astro-ph.GA2026

Evolution of Compact Stellar Systems in Ultralight Dark Matter Halos: Dependence on Stellar and Dark Matter Parameters

Yu-Ming Yang, Xiao-Jun Bi, Long Wang +1

Compact stellar systems are often used to place stringent constraints on the particle mass of ultralight dark matter (ULDM), as the heating effect induced by wave interference can…

astro-ph.CO2026

Constraints on Self-Interacting Fuzzy Dark Matter from the Stellar Kinematics of the Dwarf Galaxy Leo II

Yi Zhao, Yu-Ming Yang, Xiao-Jun Bi +1

The one-parameter fuzzy dark matter (FDM) model has faced increasingly stringent constraints from both Lyman- forest observations and local measurements of dwarf galaxies. A na…

astro-ph.CO2026

Collapse versus Disruption: The Fate of Compact Stellar Systems in Ultralight Dark Matter Halos

Yu-Ming Yang, Xiao-Jun Bi, Long Wang +1

Interference of the ultralight dark matter (ULDM) field generates time-varying gravitational potential fluctuations, which stochastically heat stellar systems embedded in ULDM halo…

hep-ph2025

Searching for Ultralight Dark Matter with M{ö}ssbauer Resonance

Peng-Long Zhang, Yu-Ming Yang, Xiao-Jun Bi +5

We investigate the feasibility of probing the interactions between ultralight scalar dark matter and atomic nuclei using a stationary Mössbauer spectroscopy scheme. The exceptiona…

astro-ph.HE2025

Probing Lorentz Invariance Violation at High Energies Using LHAASO Observations of GRB221009A via DisCan Algorithm

Yu-Chen Hua, Xiao-Jun Bi, Yu-Ming Yang +1

The Lorentz invariance violation (LIV) predicted by some quantum gravity theories would manifest as an energy-dependent speed of light, which may potentially distort the observed t…

astro-ph.CO2025

Tidal Suppression of Fuzzy Dark Matter Heating in Milky Way Satellite Galaxies

Yu-Ming Yang, Zhao-Chen Zhang, Xiao-Jun Bi +1

Many previous studies have imposed stringent constraints on the particle mass of fuzzy dark matter (FDM) by analyzing observations of Galactic satellite galaxies, which show no sig…