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Based on a hydro-inspired azimuthally symmetric emission function, we analyze the HBT radius Rs and the single-particle transverse momentum spectra in Au+Au collisions measured by the STAR Collaboration at √sNN = 200 GeV. The results show that consistent assumptions about transverse density (and/or flow profile) in the calculation of the HBT radius Rs and single-particle spectral analyses play an important role for understanding the size of the freeze-out source.
Based on a hydro-inspired azimuthally symmetric emission function, we analyze the HBT radius Rs and the single-particle transverse momentum spectra in Au + Au collisions measured by the STAR Collaboration at √sNN = 200 GeV. The results show that consistent assumptions about transverse density (and / or flow profile) in the calculation of the HBT radius Rs and single-particle spectral analyzes play an important role for understanding the size of the freeze-out source.