Extracting Information of Core Halo Model in Heavy ion Collisions by Imaging Technique
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Abstract
We characterize the spatial dimension of pionemitting source in highenergy heavy ion collisions with the radius of rootmeansquared of twopion relativedistance Rrmst. Based on the imaging technique, one can calculate Rrmst modelindependently. Applying this method to the Core-Halo model and comparing the results with that of Gaussian fitted, the results indicate that due to the effects of longlived resonance decay, the values of Rrmst show a larger spatial size of pionemitting region. Meanwhile, for the chaotic source the chaoticity factors calculated by imaging technique are larger than that of Gaussian fitted.
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