Student, Hunan University of Science and Technology, China
Shu-Peng Wang is a highly promising Undergraduate Researcher at the School of Physics and Electronics, Hunan University of Science and Technology. He has rapidly emerged as a notable young scholar in the fields of theoretical physics and astrophysics. With a deep interest in the equation of state (EoS) of dense matter, Shu-Peng authored a pioneering paper addressing thermodynamic inconsistencies in perturbative QCD by incorporating gravitational wave data such as GW170817. His work has been accepted for an international conference and showcases his expertise in theoretical modeling and numerical analysis. He has also co-authored multiple peer-reviewed publications in The European Physical Journal C, contributing to QCD and axion-related phenomena. Through collaborations with seasoned professors, he has bridged theoretical particle physics with observational astrophysics. Shu-Peng’s research trajectory reflects a rare blend of academic rigor, innovation, and ambition—making him a standout candidate for prestigious recognitions like the Best Researcher Award.
Professional Profile
Scopus | ORCID
Education
Shu-Peng Wang is currently pursuing his Bachelor’s degree in Physics at the School of Physics and Electronics, Hunan University of Science and Technology. As an undergraduate, he has already demonstrated exceptional academic and research capability, often performing at a level comparable to postgraduate scholars. His formal education has included intensive training in classical mechanics, quantum field theory, thermodynamics, and numerical simulations. Beyond coursework, he has undertaken advanced research projects in theoretical astrophysics, particularly focusing on compact stars and quantum chromodynamics (QCD). Shu-Peng’s educational journey has been enhanced by mentorship from leading physicists, including Professors Zhen-Yan Lu, Zhi-Jun Ma, and Jian-Feng Xu. This foundation has empowered him to explore the frontiers of dense matter equations of state and gravitational-wave astrophysics. His undergraduate training has laid a strong theoretical and computational groundwork, equipping him for impactful research contributions and future postgraduate studies in theoretical or computational astrophysics.
Research Focus
Shu-Peng Wang’s research centers on the theoretical and computational modeling of compact astrophysical objects, particularly quark stars. His primary interest lies in resolving thermodynamic inconsistencies in perturbative Quantum Chromodynamics (QCD) models by integrating multi-messenger astrophysical data. His work provides deeper insights into the structure and equation of state (EoS) of dense matter under extreme conditions. He has also contributed to particle physics through collaborative studies on axion properties, neutral pion decay, and topological effects in QCD at high temperatures and densities. Using tools such as SU(2) chiral perturbation theory, he investigates novel interactions that link the quantum vacuum to observable phenomena in astrophysics. His contributions demonstrate a commitment to bridging high-energy particle physics with gravitational and astrophysical observations. By combining rigorous theoretical formulations with observational constraints from events like GW170817 and GW190814, Shu-Peng’s work provides crucial advances for the understanding of neutron stars, quark matter, and exotic compact objects.
Publication Top Notes
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Constraints on the Equation of State of Quark Stars from Compact Object Observations
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Type: Conference Paper
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Date: 2025-07-29
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Authors: Shu-Peng Wang; Zhi-Jun Ma; Jian-Feng Xu; Zhen-Yan Lu
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Summary: First-authored by Shu-Peng Wang, this paper addresses a critical thermodynamic inconsistency in the perturbative QCD model. The study integrates gravitational-wave data (e.g., GW170817) to derive realistic constraints on quark star models, concluding that while two-solar-mass quark stars are viable, the massive object from GW190814 likely isn’t a simple quark star. The work bridges QCD theory with astrophysical observations.
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New Contribution to the Anomalous π0→γγ Decay in SU(2) Chiral Perturbation Theory
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Type: Conference Paper
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Date: 2025-07-28
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Authors: Zhen-Yan Lu; Shu-Peng Wang; Qi Lu
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Summary: This study provides theoretical refinements to the decay of neutral pions into two photons using SU(2) chiral perturbation theory. It includes new loop-level corrections and potential axion-induced contributions, which may impact future collider and dark matter research.
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New Axion Contribution to the Two-Photon Decays of Neutral Pions
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Type: Journal Article (The European Physical Journal C)
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Date: 2025-02-24
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Summary: Co-authored by Shu-Peng Wang, this work investigates how hypothetical axions could affect pion decay channels, potentially altering predicted decay rates and offering insight into dark sector physics and CP violation.
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QCD Topology and Axion Properties in an Isotropic Hot and Dense Medium
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Type: Journal Article (The European Physical Journal C)
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Date: 2024-11-25
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Summary: This paper explores QCD topological effects and axion behavior in high-temperature, high-density environments relevant to early universe and neutron star conditions, using theoretical simulations to assess mass and coupling constraints.
Conclusion
Given his impactful early contributions, strong theoretical foundations, and multi-disciplinary insight, Shu-Peng Wang is highly deserving of the Best Researcher Award. He exemplifies the qualities of a rising star in physics research.