EventsThe 3rd International Online Conference on Universe
Published
This submission belongs to the session S3. High Energy Nuclear and Particle Physics of the event The 3rd International Online Conference on Universe
Published date
27 Feb, 2026
Academic Editor
author-avatarMate Csanad
Citation
Chunjian Zhang, Imaging nuclear structure across energy scales: from heavy to light ions, in Proceedings of The 3rd International Online Conference on Universe, 4 March–6 March 2026, MDPI: Basel, Switzerland
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Imaging nuclear structure across energy scales: from heavy to light ions

1. Institute of Modern Physics, Fudan University, Shanghai, 200433, China, China
Abstract

Atomic nuclei are self-organized, many-body quantum systems bound by strong nuclear forces within femtometre-scale space. The shape and orientation of colliding nuclei play a crucial role in determining the initial conditions of the quark–gluon plasma (QGP), which influence key observables such as anisotropic and radial flow. In this talk, I will present an “imaging-by-smashing” approach using soft probes that are directly sensitive to the structure of colliding nuclei, from large to small systems, in high-energy nuclear collisions [1,2,3]. We present the measurements of , fluctuation, and correlations in isobar-like238U+238U and 197Au+197Au collisions at 193 and 200 GeV, respectively. Our results reveal prominent differences in these observables between the two systems, particularly in the most central collisions. We also present the first measurements of in 16O+16O and d+197Au collisions, providing insight into the impact of nucleon–nucleon correlations and further shedding light on the initial conditions of QGP droplets. Comparisons with the state-of-the-art hydrodynamic calculations enable us to extract the nuclear shape parameters across energy scales [4,5]. This interdisciplinary research enhances our understanding of the initial conditions in high-energy collisions and provides new insights into the evolution of nuclear structure across energy scales.

References:
[1] STAR Collaboration, Nature 635, 67-72 (2024)

[2] STAR Collaboration, Rep. Prog. Phys. 88, 108601 (2025)

[3] STAR Collaboration, arXiv:2510.19645

[4] C. Zhang, J. Jia, J. Chen, C. Shen, L. Liu, arXiv:2504.15245

[5] C. Zhang, J. Chen, G. Giacalone, S. Huang, J. Jia, Y.-G. Ma, PLB862, 139322(2025)

Keywords
High energy nuclear collisions
Nuclear structure
hydrodynamic models
Numerical model of the dipole phase change in Galactic Cosmic-Ray Anisotropy
About the qualities of the Schwarzschild and Generalized Schwarzschild geometries