Abstract: We present recent progress in understanding the dynamical behaviour of relativistic fluids in cosmological spacetimes. In particular, we show how the relation between expansion rate of the Universe and speed of sound of the fluid affect the stability of homogeneous fluid states.
Shock formation in cosmological fluids
03.05.2024 11:45 - 03.08.2024 13:15
Organiser:
P. Chrusciel, D. Fajman
Location: