| Issue |
EPJ Web Conf.
Volume 364, 2026
XXXI International Conference on Ultra-Relativistic Nucleus-Nucleus Collisions “Quark Matter 2025”
|
|
|---|---|---|
| Article Number | 05013 | |
| Number of page(s) | 4 | |
| Section | Correlations & Fluctuations | |
| DOI | https://doi.org/10.1051/epjconf/202636405013 | |
| Published online | 17 April 2026 | |
https://doi.org/10.1051/epjconf/202636405013
Tilted emitting source in the heavy-ion collisions
Physics Department, The Ohio State University, Columbus, Ohio 43210, USA
* e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
Published online: 17 April 2026
Abstract
The three-dimensional structure of the initial state in heavy-ion collisions has recently drawn a lot of attention. One of its key features is the tilt of the particle-emitting source away from the beam direction, which becomes more pronounced at lower collision energies. This tilt, set by the collision geometry, plays an important role in understanding observables like directed flow and particle polarization. Still, measuring the tilt directly in experiments is far from simple.
The azimuthally sensitive femtoscopy method makes it possible to study tilt by analyzing momentum correlations of pion pairs. In this work we apply it to Au+Au collisions at √sNN = 7.7 GeV. While one might expect the tilt to change mainly with centrality, our results instead show a much stronger dependence on the pair momentum.
This provides a framework that STAR can use with the ongoing high-statistics BES-II data to extract tilt more precisely and to build a clearer picture of how the three-dimensional initial state shapes final observables.
© The Authors, published by EDP Sciences, 2026
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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