About
We present the time resolved evolutions of the anisotropic flow coefficient $v_n$ with consideration of both the linear and non-linear dependence on the initial eccentricities $\epsilon_m$. The relativistic Boltzmann equation is utilized in the few collision regime in order to model the evolution of the phase space distribution. Our analytically calculated time-dependent flow harmonics are compared to results of transport simulations. Eventually, we discuss the important impact of the non-linear eccentricity contributions on the dynamical build-up of flow coefficient..
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The talk
Credits and licence
- Institution
- CERN
- Department
- Conferences
- Speaker
- Nina Kersting
- Year
- 2021
- Language
- English
- Source
- CERN
- Licence
- CERN, as CERN states it. CERN's terms
- Attribution
- © CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
- Who can watch
- CERN gives no rating. Invisible Network shows it to Teens profiles and older, judged from what the source says about it. How courses are placed