Machine-learning-based identification for initial clustering structure in relativistic heavy-ion collisions
arXiv:2109.06277 · doi:10.1103/PhysRevC.104.044902
Abstract
-clustering structure is a significant topic in light nuclei. A Bayesian convolutional neural network (BCNN) is applied to classify initial non-clustered and clustered configurations, namely Woods-Saxon distribution and three- triangular (four- tetrahedral) structure for C (O), from heavy-ion collision events generated within a multi-phase transport (AMPT) model. Azimuthal angle and transverse momentum distributions of charged pions are taken as inputs to train the classifier. On multiple-event basis, the overall classification accuracy can reach for C/O + Au events at 200 GeV. With proper constructions of samples, the predicted deviations on mixed samples with different proportions of both configurations could be within . In addition, setting a simple confidence threshold can further improve the predictions on the mixed dataset. Our results indicate promising and extensive possibilities of application of machine-learning-based techniques to real data and some other problems in physics of heavy-ion collisions.
arXiv comment12 pages, 11 figures; Accepted by Physical Review C
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