2008/01/31 by M. Csanád, Mate Csanad, Boris Tomášik +3 · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #High-Energy Particle Collisions Research #Quantum Chromodynamics and Particle Interactions #nucl-th
paper · pdf · doi:10.1140/epja/i2008-10605-7
published as Eur.Phys.J.A37:111-119,2008 · 7 pages, 4 figures, prepared with svjour.cls, accepted at Eur. Phys. J. A
arxiv created 2008/06/12 · openalex publication_date 2008/07/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present a calculation of the elliptic flow and azimuthal dependence of the correlation radii in the ellipsoidally symmetric generalization of the Buda-Lund model. The elliptic flow is shown to depend only on the flow anisotropy while in case of correlation radii both flow and space anisotropy play an important role in determining their azimuthal oscillation. We also outline a simple procedure for determining the parameters of the model from data.