| Speaker | Saumia Pandiat Sankar, Institute of Physics, Bhubaneswar, India and GPP, UdeM, Montréal |
|---|---|
| Date | Friday, May 14, 2010, 3:00 PM |
| Location | Roger Gaudry, V-221 |
Abstract
We show that there are crucial similarities in the physics of cosmic microwave background radiation (CMBR) anisotropies and the flow anisotropies in relativistic heavy-ion collision experiments (RHICE). We also argue that, following CMBR anisotropy analysis, a plot of root-mean square values of the flow coefficients, calculated in a lab fixed frame for RHICE, can yield important information about the nature of initial state anisotropies and their evolution.
Refreshments will be served at café et biscuits à 10h30, au V-221.
