activity
20082026
most citedConstraints on Lorentz invariance violation from the LHAASO observation of GRB 221009A

18 citations · 81 across the 31 of their papers we have counts for

collaborators

33 papers

astro-ph.CO2026

Dynamics of Wave Structures in Multifield Fuzzy Dark Matter Halos

Yu-Ming Yang, Xiao-Jun Bi, Peng-Fei Yin

As a natural extension of the single-field fuzzy dark matter (FDM) model, multifield FDM has attracted increasing attention in recent years. This scenario is motivated both by the…

hep-ph2026

Sideband Structure of Axion Electrodynamics

Run-Min Yao, Xiao-Jun Bi, Peng-Fei Yin +1

We develop a Floquet--Bloch sideband formulation of the linearized Maxwell--axion system in a coherent periodic axion background. Linearizing around prescribed magnetic and axion f…

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 nat…

astro-ph.HE2026

Diverse properties of electron Forbush decreases revealed by the Dark Matter Particle Explorer

F. Alemanno, Q. An, P. Azzarello +147

The Forbush decrease (FD) of cosmic rays is an important probe of the interplanetary environment disturbed by solar activities. In this work, we study the properties of 8 FDs elect…

hep-ph2026

Resonant photon-axion conversion driven by axion dark matter oscillations

Run-Min Yao, Xiao-Jun Bi, Peng-Fei Yin +1

Wave propagation in periodically time-dependent media can exhibit driven mode conversion that is absent in static or adiabatic descriptions. We show that coherent axion dark matter…

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 exceptional…

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★ 7 cited

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…

hep-ph2025

Axion-like Dark Matter Search with Space-based Gravitational Wave Detectors

Run-Min Yao, Xiao-Jun Bi, Peng-Fei Yin +1

We propose a novel modification to the optical benches of space-based gravitational wave detectors (SGWDs) to enable the detection of axion-like dark matter (ALDM)-induced birefrin…

hep-ph2025★ 10 cited

Constraints on Lorentz-invariance violation in the neutrino sector from the ultrahigh-energy event KM3-230213A

Yu-Ming Yang, Xing-Jian Lv, Xiao-Jun Bi +1

Lorentz invariance is a fundamental symmetry of spacetime and serves as the cornerstone of modern physics, supporting the constancy of the speed of light. A crucial implication of…

astro-ph.HE2025

Exploring Constraints on Axion-like Particles with the Observations for blazar Mrk 501

Ting Zhou, Lin-Qing Gao, Xiao-Jun Bi +2

Oscillations between axion-like particles (ALPs) and photons in astrophysical magnetic fields can lead to irregularities in the high energy gamma ray spectra of blazars. The magnet…

astro-ph.CO2024★ 2 cited

Construction of fuzzy dark matter halos with arbitrary initial velocities

Yu-Ming Yang, Xiao-Jun Bi, Peng-Fei Yin

Cosmological simulations of fuzzy dark matter (FDM) are computationally expensive, and the resulting halos lack flexibility in parameter adjustments, such as virial mass, density p…

astro-ph.GA2024★ 4 cited

Interpreting the Extremely Diffuse Stellar Distribution of the Nube Galaxy through Fuzzy Dark Matter

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

Recent observations have uncovered a remarkably flat and extremely diffuse stellar distribution within the almost dark dwarf galaxy Nube, posing a challenge to the standard cold da…

hep-ph2024

SKA Sensitivity to Potential Radio Emission from Dark Matter Annihilation in Ursa Major III

Peng-Long Zhang, Xiao-Jun Bi, Qin Chang +2

The recently discovered stellar system, Ursa Major III/UNIONS 1, may be the faintest and densest dwarf spheroidal satellite galaxy of the Milky Way. Owing to its close proximity an…

astro-ph.CO2024

Reproduction of NGC1052-DF4 by self-interacting dark matter: dark matter deficiency and tidal features

Zhao-Chen Zhang, Xiao-Jun Bi, Peng-Fei Yin

Observations of the velocity dispersion indicate a severe dark matter (DM) deficit in the ultra-diffuse galaxy, NGC1052-DF4 (DF4). The ultra-deep images obtained with the Gemini te…

astro-ph.HE2024

Impact of Parameters in the Blazar Jet Magnetic Field Model on Axion-Like Particle Constraints

Lin-Qing Gao, Xiao-Jun Bi, Jun Li +1

The interaction between axion-like particles (ALPs) and photons induces ALP-photon oscillations in astrophysical magnetic fields, leading to spectral distortions in the -ray spe…

astro-ph.HE2024

Determination of dark matter distribution in Ursa Major III and constraints on dark matter annihilation

Yi Zhao, Xiao-Jun Bi, Su-Jie Lin +1

The recently discovered satellite dwarf galaxy Ursa Major III provides a promising opportunity to explore the signatures resulting from dark matter (DM) annihilation, due to its pr…

astro-ph.CO2024

A theoretical perspective on the almost dark galaxy Nube: exploring the fuzzy dark matter model

Yu-Ming Yang, Xiao-Jun Bi, Peng-Fei Yin

In recent astronomical observations, an almost dark galaxy, designated as Nube, has unveiled an intriguing anomaly in its stellar distribution. Specifically, Nube exhibits an excep…

astro-ph.HE2024

Precise measurement of the cosmic-ray spectrum and by LHAASO -- connecting the Galactic to the extragalactic components

Xing-Jian Lv, Xiao-Jun Bi, Kun Fang +6

Recently LHAASO Collaboration gives precise measurements of cosmic rays (CR) all particle energy spectrum and mean logarithmic mass from 0.3 Pe…

astro-ph.CO2024★ 1 cited

Tidal Formation of dark matter deficit diffuse galaxy NGC1052-DF2 by SIDM

Zhao-Chen Zhang, Xiao-Jun Bi, Peng-Fei Yin

Observations have revealed a significant dark matter deficit in the ultra-diffuse galaxy NGC1052-DF2 (DF2). It is widely accepted that the formation of this unique galaxy can be at…

astro-ph.HE2024

Interpretation of AMS-02 beryllium isotope fluxes using data-driven production cross sections

Meng-Jie Zhao, Xiao-Jun Bi, Kun Fang +1

The Be isotopic measurements preliminarily reported by the AMS-02 Collaboration have reached an unprecedented energy of 12 GeV/. As secondary cosmic rays (CRs), the Be isotopes…

astro-ph.HE2024★ 1 cited

Possible spectral irregularities in the AMS-02 positron spectrum

Xing-Jian Lv, Xiao-Jun Bi, Kun Fang +2

The excesses in the electron and positron spectra observed by many experiments, such as PAMELA and AMS-02, have sparked significant theoretical investigation. It is not easy to dis…