pith. sign in

arxiv: nucl-ex/0605032 · v1 · submitted 2006-05-25 · ⚛️ nucl-ex

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
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Pion emission source shape in UrQMD Au+Au collisions at STAR energies

    nucl-th 2026-05 unverdicted novelty 4.0

    UrQMD simulations show pion source radii increasing with collision energy and decreasing with transverse mass, with the Levy index alpha falling at higher energies.