Abstract
We investigate interaction dependence of the intensity correlation in high-energy heavy-ion collisions. By analyzing the correlation data recently obtained by the STAR collaboration based on theoretically proposed interactions, we give a constraint on the scattering length, , suggesting that interaction is weakly attractive and there is no loosely bound state. In addition to the fermionic quantum statistics and the interaction, effects of collective flow, feed-down from , and the residual source are also found to be important to understand the data. We demonstrate that the correlation data favor negative scattering length with the pair purity parameter evaluated by using experimental data on the ratio, while the positive scattering length could be favored when we regard as a free fitting parameter.
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