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4 - Simulating Relativistic Nuclear Collisions

Published online by Cambridge University Press:  29 April 2019

Paul Romatschke
Affiliation:
University of Colorado Boulder
Ulrike Romatschke
Affiliation:
National Center for Atmospheric Research, Boulder, Colorado
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Summary

This chapter reviews the basic ingredients of simulating relativistic nuclear collisions, of which fluid dynamics is one component. Nuclear geometry models with and without subnucleonic degrees of freedom are discussed, energy deposition at weak and strong coupling is reviewed and found to lead to similar results as the simple Glauber model with number of collision scaling. Initial state eccentricities are calculated, numerical algorithms to solve relativistic dissipative fluid dynamics are discussed and the freeze-out from fluid to particle degrees of freedom (hadronization) is described. The chapter closes with a discussion on how to calculate relevant observables in relativistic nuclear collision experiments.

Type
Chapter
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Relativistic Fluid Dynamics In and Out of Equilibrium
And Applications to Relativistic Nuclear Collisions
, pp. 96 - 143
Publisher: Cambridge University Press
Print publication year: 2019

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