arXiv · 1311.0999
Non-equilibrium phase transition in relativistic nuclear collisions: Importance of the equation of state
Abstract
Within the context of relativistic nuclear collisions aimed at exploring hot and baryon-dense matter, we investigate how the general features of the expansion dynamics, as well as a number of specific observables, depend on the equation of state used in dynamical simulations of the non-equilibrium confinement phase transition.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Jan Steinheimer, Jørgen Randrup, Volker Koch. 2014-03-07. Non-equilibrium phase transition in relativistic nuclear collisions: Importance of the equation of state. https://doi.org/10.1103/physrevc.89.034901
Cite the original work for its findings. Save a collection to share your selection of sources.