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Beam energy dependence of rapidity-even dipolar flow in Au+Au collisions

MPS-Authors

STAR Collaboration, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Adam,  J.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Schmitz,  N.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Seyboth,  P.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

et al., 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

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Citation

STAR Collaboration, Adam, J., Schmitz, N., Seyboth, P., & et al. (2018). Beam energy dependence of rapidity-even dipolar flow in Au+Au collisions. Physics Letters B, (784), 26-32. Retrieved from https://publications.mppmu.mpg.de/?action=search&mpi=MPP-2018-313.


Cite as: https://hdl.handle.net/21.11116/0000-0003-F94D-F
Abstract
New measurements of directed flow for charged hadrons, characterized by the Fourier coefficient \vone, are presented for transverse momenta $\mathrm{p_T}$, and centrality intervals in Au+Au collisions recorded by the STAR experiment for the center-of-mass energy range $\mathrm{\sqrt{s_{_{NN}}}} = 7.7 - 200$ GeV. The measurements underscore the importance of momentum conservation and the characteristic dependencies on $\mathrm{\sqrt{s_{_{NN}}}}$, centrality and $\mathrm{p_T}$ are consistent with the expectations of geometric fluctuations generated in the initial stages of the collision, acting in concert with a hydrodynamic-like expansion. The centrality and $\mathrm{p_T}$ dependencies of $\mathrm{v^{even}_{1}}$, as well as an observed similarity between its excitation function and that for $\mathrm{v_3}$, could serve as constraints for initial-state models. The $\mathrm{v^{even}_{1}}$ excitation function could also provide an important supplement to the flow measurements employed for precision extraction of the temperature dependence of the specific shear viscosity.