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Title: | Anisotropic flow fluctuation as a possible signature of clustered nuclear geometry in O–O collisions at the Large Hadron Collider |
Authors: | Prasad, Suraj k Mallick, Neelkamal Sahoo, Raghunath |
Issue Date: | 2025 |
Publisher: | Elsevier B.V. |
Citation: | Prasad, S., Mallick, N., Sahoo, R., & Barnaföldi, G. G. (2025). Anisotropic flow fluctuation as a possible signature of clustered nuclear geometry in O–O collisions at the Large Hadron Collider. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. Scopus. https://doi.org/10.1016/j.physletb.2024.139145 |
Abstract: | Nuclei having 4n number of nucleons are theorized to possess clusters of α particles (4He nucleus). The Oxygen nucleus (16O) is a doubly magic nucleus, where the presence of an α-clustered nuclear structure grants additional nuclear stability. In this study, we exploit the anisotropic flow coefficients to discern the effects of an α-clustered nuclear geometry with respect to a Woods-Saxon nuclear distribution in O–O collisions at sNN=7 TeV using a hybrid of IP-Glasma + MUSIC + iSS + UrQMD models. In addition, we use the multi-particle cumulants method to measure anisotropic flow coefficients, such as elliptic flow (v2) and triangular flow (v3), as a function of multiplicity class. Anisotropic flow fluctuations, which are expected to be larger in small collision systems, are also studied for the first time in O–O collisions. It is found that an α-clustered nuclear distribution gives rise to an enhanced value of v2 and v3 for the low-multiplicity events. Consequently, a rise in v3/v2 is also observed for the 0–10% multiplicity class. Further, for α-clustered O–O collisions, fluctuations of v2 are larger for the highest multiplicity events, which decrease as the final-state multiplicity decreases. In contrast, for a Woods-Saxon 16O nucleus, v2 fluctuations show an opposite behavior with decreasing multiplicity. When confronted with experimental data, this study may reveal the importance of the nuclear density profile on the discussed observables and provide physics validation for the hybrid model discussed in this work. © 2024 The Author(s) |
URI: | https://doi.org/10.1016/j.physletb.2024.139145 https://dspace.iiti.ac.in/handle/123456789/15109 |
ISSN: | 0370-2693 |
Type of Material: | Journal Article |
Appears in Collections: | Department of Physics |
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