Xiao-Jun Bi

8.0k total citations
150 papers, 2.4k citations indexed

About

Xiao-Jun Bi is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Statistical and Nonlinear Physics. According to data from OpenAlex, Xiao-Jun Bi has authored 150 papers receiving a total of 2.4k indexed citations (citations by other indexed papers that have themselves been cited), including 132 papers in Nuclear and High Energy Physics, 79 papers in Astronomy and Astrophysics and 6 papers in Statistical and Nonlinear Physics. Recurrent topics in Xiao-Jun Bi's work include Dark Matter and Cosmic Phenomena (117 papers), Particle physics theoretical and experimental studies (73 papers) and Cosmology and Gravitation Theories (62 papers). Xiao-Jun Bi is often cited by papers focused on Dark Matter and Cosmic Phenomena (117 papers), Particle physics theoretical and experimental studies (73 papers) and Cosmology and Gravitation Theories (62 papers). Xiao-Jun Bi collaborates with scholars based in China, United States and Italy. Xiao-Jun Bi's co-authors include Peng‐Fei Yin, Qiang Yuan, Xinmin Zhang, Zhao-Huan Yu, Kun Fang, Sujie Lin, Pei-Hong Gu, Juan Zhang, Qian-Fei Xiang and Qi-Shu Yan and has published in prestigious journals such as Physical Review Letters, SHILAP Revista de lepidopterología and The Astrophysical Journal.

In The Last Decade

Xiao-Jun Bi

140 papers receiving 2.3k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
Xiao-Jun Bi China 29 2.2k 1.3k 115 105 19 150 2.4k
Luca Maccione Italy 20 1.0k 0.5× 628 0.5× 82 0.7× 185 1.8× 17 0.9× 37 1.1k
Yosuke Mizuno Germany 24 1.3k 0.6× 1.7k 1.2× 48 0.4× 48 0.5× 17 0.9× 97 1.8k
Da-Ming Wei China 20 538 0.2× 1.3k 1.0× 31 0.3× 30 0.3× 9 0.5× 96 1.4k
A. Yu. Smirnov Italy 35 4.3k 1.9× 512 0.4× 125 1.1× 81 0.8× 8 0.4× 93 4.3k
Marco Drewes Belgium 21 1.6k 0.7× 695 0.5× 99 0.9× 75 0.7× 2 0.1× 49 1.8k
G. Fossati United States 18 2.5k 1.1× 2.4k 1.8× 30 0.3× 12 0.1× 15 0.8× 25 2.6k
M. Ajello United States 27 1.8k 0.8× 2.2k 1.6× 57 0.5× 17 0.2× 9 0.5× 120 2.5k
C. Ferrari France 22 466 0.2× 1.2k 0.9× 79 0.7× 27 0.3× 12 0.6× 66 1.4k
T. Kajita Japan 22 1.7k 0.8× 255 0.2× 83 0.7× 33 0.3× 9 0.5× 62 1.8k
Matthew Bainbridge United States 10 184 0.1× 363 0.3× 132 1.1× 47 0.4× 5 0.3× 15 559

Countries citing papers authored by Xiao-Jun Bi

Since Specialization
Citations

This map shows the geographic impact of Xiao-Jun Bi's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Xiao-Jun Bi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Xiao-Jun Bi more than expected).

Fields of papers citing papers by Xiao-Jun Bi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Xiao-Jun Bi. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by Xiao-Jun Bi. The network helps show where Xiao-Jun Bi may publish in the future.

Co-authorship network of co-authors of Xiao-Jun Bi

This figure shows the co-authorship network connecting the top 25 collaborators of Xiao-Jun Bi. A scholar is included among the top collaborators of Xiao-Jun Bi based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Xiao-Jun Bi. Xiao-Jun Bi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Bi, Xiao-Jun, et al.. (2025). A Rigorous Solution to the Superluminal Issue in the Diffusion Equation. The Astrophysical Journal. 982(2). 85–85. 1 indexed citations
2.
Bi, Xiao-Jun, et al.. (2025). Prediction of lithium isotope fluxes using data-driven production cross sections. Physical review. D. 112(4).
3.
Bi, Xiao-Jun, Kun Fang, Yi-Qing Guo, et al.. (2025). Precise Measurement of the Cosmic-Ray Spectrum and 〈ln A〉 by LHAASO: Connecting the Galactic to the Extragalactic Components. The Astrophysical Journal. 979(2). 225–225. 1 indexed citations
4.
Bi, Xiao-Jun, et al.. (2025). Reproduction of NGC1052-DF4 by self-interacting dark matter: dark matter deficiency and tidal features. Journal of Cosmology and Astroparticle Physics. 2025(3). 31–31. 2 indexed citations
5.
Bi, Xiao-Jun, et al.. (2025). Interpreting the Extremely Diffuse Stellar Distribution of the Nube Galaxy through Fuzzy Dark Matter. The Astrophysical Journal Letters. 981(2). L26–L26. 1 indexed citations
6.
Bi, Xiao-Jun, et al.. (2025). Insights into improved chloride resistance of carbon steel in Portland cement blended with belitic calcium sulfoaluminate cement. Cement and Concrete Composites. 165. 106327–106327.
7.
Bi, Xiao-Jun, et al.. (2024). Constraints on Lorentz invariance violation from the LHAASO observation of GRB 221009A. Journal of Cosmology and Astroparticle Physics. 2024(4). 60–60. 7 indexed citations
8.
Bi, Xiao-Jun, et al.. (2024). Cosmic-ray deuteron excess from a primary component. Physical review. D. 110(12). 1 indexed citations
9.
Li, Jun, et al.. (2024). Constraints on axion-like particles from the observation of Galactic sources by the LHAASO*. Chinese Physics C. 48(6). 65107–65107. 4 indexed citations
10.
Fang, Kun, et al.. (2023). Effect of the magnetic field correlation length on the gamma-ray pulsar halo morphology under anisotropic diffusion. Physical review. D. 108(2). 3 indexed citations
11.
Fang, Kun, et al.. (2022). Features of the gamma-ray pulsar halo HESS J1831098. Physical review. D. 106(12). 5 indexed citations
12.
Fang, Kun, et al.. (2022). Slow Diffusion is Necessary to Explain the γ-Ray Pulsar Halos. The Astrophysical Journal. 936(2). 183–183. 14 indexed citations
13.
Fang, Kun & Xiao-Jun Bi. (2022). Interpretation of the puzzling gamma-ray spectrum of the Geminga halo. Physical review. D. 105(10). 6 indexed citations
14.
Bi, Xiao-Jun, et al.. (2021). Exploring axion dark matter through radio signals from magnetic white dwarf stars. Physical review. D. 103(11). 12 indexed citations
15.
Wang, Shenghao, Kun Fang, Xiao-Jun Bi, & Peng‐Fei Yin. (2021). Test of the superdiffusion model in the interstellar medium around the Geminga pulsar. Physical review. D. 103(6). 10 indexed citations
16.
Fang, Kun, Shao-Qiang Xi, & Xiao-Jun Bi. (2021). Self-consistent interpretations of the multiwavelength gamma-ray spectrum of LHAASO J0621+3755. Physical review. D. 104(10). 10 indexed citations
17.
Rui, Qi, Shangyi Fu, Qingnan Liang, et al.. (2021). A novel stop codon mutation of TSPAN12 gene in Chinese patients with familial exudative vitreoretinopathy. Ophthalmic Genetics. 43(2). 210–217. 1 indexed citations
18.
Bi, Xiao-Jun, Peng‐Fei Yin, Zhao-Huan Yu, & Qiang Yuan. (2011). Constraints and tests of the superluminal neutrinos at OPERA. arXiv (Cornell University). 7 indexed citations
19.
Gu, Pei-Hong & Xiao-Jun Bi. (2004). Leptogenesis with triplet Higgs boson. arXiv (Cornell University). 3 indexed citations
20.
Bi, Xiao-Jun, Mingzhe Li, & Xinmin Zhang. (2003). Quintessino as Dark Matter. arXiv (Cornell University). 3 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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