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Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt sNN=200 GeV
S S Adler1, S Afanasiev, C Aidala
1Brookhaven National Laboratory, Upton, New York 11973-5000, USA.
Abstract:
Emission source functions are extracted from correlation functions constructed from charged pions produced at midrapidity in Au+Au collisions at sqrt[s(NN)]=200 GeV. The source parameters extracted from these functions at low k(T) give first indications of a long tail for the pion emission source. The source extension cannot be explained solely by simple kinematic considerations. The possible role of a halo of secondary pions from resonance emissions is explored.
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