Abstract
In this talk, we report an analysis of elliptic flow (v2), non-flow (δ2) and v2 fluctuations for the STAR Collaboration at middle rapidity in GeV Au+Au collisions. We compare the results to models of the fluctuations in the initial eccentricity of the overlap zone.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
More From: Journal of Physics G: Nuclear and Particle Physics
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.