Abstract
It is important to understand whether \(\alpha \)-clustering structures can leave traces in ultra-relativistic heavy ion collisions. Using the modified AMPT model, we simulate three \(\alpha \) + core configurations of \(^{44}\)Ti in \(^{44}\)Ti\( +^{44}\)Ti collisions at \(\sqrt{s_{NN}}=5.02\) TeV as well as other systems with Woods-Saxon structures. One of these configurations has no additional constraint, but the other two have the Mott density edge \(r_{\textrm{Mott}}\) set as either a lower or upper bound on the cluster position \(r_{\alpha }\) to check the influence of \(\alpha \) dissolution. This is the first time that the initial stage of the geometric properties in heavy-ion collisions has been configured using the traditional treatment of the nuclear structure. We compare the radial nucleon density, multiplicity distribution, transverse momentum spectra, eccentricity, triangularity, elliptic flow and triangular flow of these six systems. \(\alpha +\) core structures can alter all these observations especially in the most-central collisions, among which elliptic flow is the most hopeful as a probe of such structures.
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This manuscript has no associated data or the data will not be deposited. [Authors’ comment: xxx.].
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Acknowledgements
This work was supported in part by National Key R &D Program of China under Grant No. 2018YFE0104600 and 2016YFE0100900, the National Natural Science Foundation of China under contract Nos. 12275054, 11890710, 11890714, 11925502, 12147101, 12061141008 and 11875066, the Strategic Priority Research Program of CAS under Grant No. XDB34000000, the Guangdong Major Project of Basic and Applied Basic Research No. 2020B0301030008, Shanghai Special Project for Basic Research No. 22TQ006 and the STCSM under Grant No. 23590780100.
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Zhang, YX., Zhang, S. & Ma, YG. Signatures of an \(\alpha \) + core structure in \(^{44}\)Ti + \(^{44}\)Ti collisions at \(\sqrt{s_{NN}}=5.02\) TeV by a multiphase transport model. Eur. Phys. J. A 60, 73 (2024). https://doi.org/10.1140/epja/s10050-024-01290-x
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DOI: https://doi.org/10.1140/epja/s10050-024-01290-x