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We discuss the use of the hydrodynamic model for the description of theevolution of dense matter formed in ultrarelativistic heavy-ion collisions. Thecollective flow observed in heavy-ion collisions at the BNL Relativistic HeavyIon Collider and at the CERN Large Hadron Collider is consistent with theassumption that a fireball of strongly interacting matter is formed.Experimental results from p-Pb and d-Au collisions show similar phenomena,which suggests that collective expansion appears in small systems as well. Wereview the recent application of the hydrodynamic model to small systems anddiscuss limitations and possible further checks of this scenario.

Hydrodynamic models of ultrarelativistic collisions