Published July 30, 2014 | Version v1
Journal article

How (non-)linear is the hydrodynamics of heavy ion collisions?

  • 1. Physics Department, Theory Unit, CERN, CH-1211 Genève 23 (Switzerland)
  • 2. Dep. de Fisica de Particulas, U. de Santiago de Compostela, E-15782 Santiago de Compostela, Galicia (Spain)
  • 3. INAF - Osservatorio Astrofisico di Arcetri, L.go E. Fermi 5, I-50125 Firenze (Italy)
  • 4. INFN - Sezione di Firenze, Via G. Sansone 1, I-50019 Sesto F.no (Firenze) (Italy)
  • 5. Dipartimento di Fisica e Astronomia, Università di Firenze, Via G. Sansone 1, I-50019 Sesto F.no (Firenze) (Italy)
  • 6. Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, I-44100 Ferrara (Italy)
  • 7. INFN - Sezione di Ferrara, Via Saragat 1, I-44100 Ferrara (Italy)

Description

We provide evidence from full numerical solutions that the hydrodynamical evolution of initial density fluctuations in heavy ion collisions can be understood order-by-order in a perturbative series in deviations from a smooth and azimuthally symmetric background solution. To leading linear order, modes with different azimuthal wave numbers do not mix. When quadratic and higher order corrections are numerically sizable, they can be understood as overtones with corresponding wave numbers in a perturbative series. Several findings reported in the recent literature result naturally from the general perturbative series formulated here

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2014.06.049

Additional details

Identifiers

DOI
10.1016/j.physletb.2014.06.049;
arXiv
arXiv:1312.5482v1;
PII
S0370-2693(14)00454-7;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
735
Journal Issue
Complete
Journal Page Range
p. 305-310
ISSN
0370-2693
CODEN
PYLBAJ

INIS

Optional Information

Copyright
Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.