Evidence for a long-range component in the pion emission source in Au+Au collisions at sqrt(s_NN) = 200 GeV
classification
⚛️ nucl-ex
keywords
sourceemissionfunctionscollisionsextractedpionpionssqrt
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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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Forward citations
Cited by 1 Pith paper
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Pion emission source shape in UrQMD Au+Au collisions at STAR energies
UrQMD simulations show pion source radii increasing with collision energy and decreasing with transverse mass, with the Levy index alpha falling at higher energies.
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