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      Fluctuations around Bjorken Flow and the onset of turbulent phenomena

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          Abstract

          We study how fluctuations in fluid dynamic fields can be dissipated or amplified within the characteristic spatio-temporal structure of a heavy ion collision. The initial conditions for a fluid dynamic evolution of heavy ion collisions may contain significant fluctuations in all fluid dynamical fields, including the velocity field and its vorticity components. We formulate and analyze the theory of local fluctuations around average fluid fields described by Bjorken's model. For conditions of laminar flow, when a linearized treatment of the dynamic evolution applies, we discuss explicitly how fluctuations of large wave number get dissipated while modes of sufficiently long wave-length pass almost unattenuated or can even be amplified. In the opposite case of large Reynold's numbers (which is inverse to viscosity), we establish that (after suitable coordinate transformations) the dynamics is governed by an evolution equation of non-relativistic Navier-Stokes type that becomes essentially two-dimensional at late times. One can then use the theory of Kolmogorov and Kraichnan for an explicit characterization of turbulent phenomena in terms of the wave-mode dependence of correlations of fluid dynamic fields. We note in particular that fluid dynamic correlations introduce characteristic power-law dependences in two-particle correlation functions.

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          Most cited references12

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          Anisotropy as a signature of transverse collective flow

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            Viscosity Information from Relativistic Nuclear Collisions: How Perfect is the Fluid Observed at RHIC?

            Relativistic viscous hydrodynamic fits to RHIC data on the centrality dependence of multiplicity, transverse and elliptic flow for sqrt{s}=200 GeV Au+Au collisions are presented. For Glauber-type initial conditions, while data on integrated v_2 is consistent with a ratio of viscosity over entropy density up to eta/s=0.16, data on minimum bias v_2 seems to favor a much smaller viscosity over entropy ratio, below the bound from the AdS/CFT conjecture. Some caveats on this result are discussed.
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              A Hydrodynamic Description of Heavy Ion Collisions at the SPS and RHIC

              A hydrodynamic + cascade model of relativistic heavy ion collisions is presented and compared to available hadronic data from the SPS to RHIC. The model consistently reproduces the radial and elliptic flow data for different particles, collision energies, and impact parameters. Three ingredients are essential to the success: (a) a reasonable EOS exhibiting the hard and soft features of the QCD phase transition, (b) thermal hadronization at the phase boundary, and (c) subsequent hadronic rescattering. Some features of the RHIC data are readily explained: (i) the observed elliptic flow and its dependence on \(p_{T}\) and mass, (ii) the anomalous \(\bar{p}/\pi^{-}\) ratio for \(p_{T} \approx 2.0\) GeV, (iii) the difference in the slope parameters measured by the STAR and PHENIX collaborations, and (iv) the respectively strong and weak impact parameter dependence of the \(\bar{p}\) and \(\phi\) slope parameters. For an EOS without the hard and soft features of the QCD phase transition, the broad consistency with the data is lost.
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                Author and article information

                Journal
                29 August 2011
                2012-08-17
                Article
                10.1007/JHEP11(2011)100
                1108.5535
                9897f9e7-19a6-4a9d-a04f-89fefdda382e

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                CERN-PH-TH/2011-213
                JHEP 11, 100 (2011)
                40 pages, 5 figures, published version
                nucl-th hep-ph

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