Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt(s_NN) = 200 GeV

Details Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt(s_NN) = 200 GeV Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt(s_NN) = 200 GeV

2006-05-25

arxiv.org/abs/nucl-ex/0605032v1

Phys.Rev.Lett.98:132301,2007

Physics

Nuclear Physics

Nuclear Experiment

334 authors, 6 pages, 3 figures, no tables. Submitted to Phys. Rev. Lett. Plain text data tables for the points plotted in fig

Scientific paper

10.1103/PhysRevLett.98.132301

Emission source functions are extracted from correlation functions constructed from charged pions produced at mid-rapidity 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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