Abstract
We investigate the correlation between various aspects of the initial geometry of heavy ion collisions at the BNL Relativistic Heavy Ion Collider energies and the final anisotropic flow, using v-USPhydro, a event-by-event viscous relativistic hydrodynamical model. We test the extent of which shear and bulk viscosity affect the prediction of the final flow harmonics, , from the initial eccentricities, . We investigate in detail the flow harmonics through where we find that , and are dependent on more complicated aspects of the initial geometry that are especially important for the description of peripheral collisions, including a nonlinear dependence on eccentricities as well as a dependence on shorter-scale features of the initial density. Furthermore, we compare our results to previous results from NeXSPheRIO, a relativistic ideal hydrodynamical model that has a nonzero initial flow contribution, and find that the combined contribution from dynamics and nonzero, fluctuating initial flow decreases the predictive ability of the initial eccentricities, in particular for very peripheral collisions, but also disproportionately in central collisions.
4 More- Received 11 November 2014
- Revised 14 January 2015
DOI:https://doi.org/10.1103/PhysRevC.91.034902
©2015 American Physical Society