Document Type
Article
Publication Date
2012
DOI
10.1103/PhysRevC.86.014904
Publication Title
Physical Review C
Volume
86
Issue
1
Pages
014904 (1-15)
Abstract
We present STAR measurements of azimuthal anisotropy by means of the two- and four-particle cumulants ν2 ν2{2} and ν2{4}) for Au + Au and Cu + Cu collisions at center-of-mass energies √ˢᴺᴺ = 62.4 and 200 GeV. The difference between ν2{2}2 and ν2{4}2 is related to ν2fluctuations (σν2) and nonflow (δ2). We present an upper limit to σν2/ν2. Following the assumption that eccentricity fluctuations σε dominate ν2 fluctuations σν2/ν2 ≈ σε/ε we deduce the nonflow implied for several models of eccentricity fluctuations that would be required for consistency with ν2{2} and ν2{4}. We also present results on the ratio of ν2 to eccentricity.
Original Publication Citation
Agakishiev, G., Aggarwal, M. M., Ahammed, Z., Alakhverdyants, A. V., Alekseev, I., Alford, J., . . . Zoulkarneeva, Y. (2012). Energy and system size dependence of two- and four-particle ν2 measurements in heavy-ion collisions at √ˢᴺᴺ = 62.4 and 200 GeV and their implications on flow fluctuations and nonflow. Physical Review C, 86(1), 014904. doi:10.1103/PhysRevC.86.014904
Repository Citation
Agakishiev, G.; Aggarwal, M. M.; Ahammed, Z.; Alakhverdyants, A. V.; Bueltmann, M.; and STAR Collaboration, "Energy and System Size Dependence of Two- and Four-Particle ν2 Measurements in Heavy-Ion Collisions at √ˢᴺᴺ = 62.4 and 200 GeV and Their Implications on Flow Fluctuations and Nonflow" (2012). Physics Faculty Publications. 168.
https://digitalcommons.odu.edu/physics_fac_pubs/168
Comments
"Yes, the author or the author's employer may use all or part of the APS published article, including the APS-prepared version (e.g., the PDF from the online journal) without revision or modification, on the author's or employer's website as long as a fee is not charged. If a fee is charged, then APS permission must be sought. In all cases, the appropriate bibliographic citation and notice of the APS copyright must be included."
© American Physical Society