Opening book details…
Can I read Beam-energy and collision-system dependence of the linear and mode-coupled flow harmonics from STAR on EtoBox?
Beam-energy and collision-system dependence of the linear and mode-coupled flow harmonics from STAR by Magdy, Niseem is a Physics and Astronomy article available to read on EtoBox.
What is Beam-energy and collision-system dependence of the linear and mode-coupled flow harmonics from STAR about?
Recent measurements and hydrodynamic model calculations suggest that the higher-order flow coefficients v 4 and v 5 have two contributions: a linear contribution driven by the initial-state eccentricities, ε n , and a mode-coupled contribution derived from the lower-order eccentricity coefficients ε 2 and ε 3 . Measurements of these two contributions to v 4 and v 5 provide crucial insights to discern initial-state models and to constrain the temperature-dependent specific shear viscosity, η/s, of the plasma produced in heavy-ion collisions. In this work, we have employed the two-subevents cumulant technique to provide the first beam-energy and collision-system dependence of the linear and mode-coupled contributions to the higher-order flow harmonics. Our results are shown and discussed for several centrality intervals for U+U collisions at √ s NN = 193 GeV, Au+Au collisions at √ s NN =200, and 54.4 GeV and Cu+Au collisions at √ s NN =200 GeV. The results are compared with similar studies performed by the ALICE experiment at LHC.
Who reads Beam-energy and collision-system dependence of the linear and mode-coupled flow harmonics from STAR?
It is typically read by researchers, students, and practitioners in Physics and Astronomy.
- Author
- Magdy, Niseem
- Publisher
- Elsevier Science; Elsevier ; Elsevier BV (ISSN 0375-9474)
- Published
- 2021
- Language
- EN
- Field
- Physics and Astronomy (Physical Sciences)