2015
DOI: 10.1007/jhep12(2015)067
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Scaling relations in two-dimensional relativistic hydrodynamic turbulence

Abstract: We derive exact scaling relations for two-dimensional relativistic hydrodynamic turbulence in the inertial range of scales. We consider both the energy cascade towards large scales and the enstrophy cascade towards small scales. We illustrate these relations by numerical simulations of turbulent weakly compressible flows. Intriguingly, the fluid-gravity correspondence implies that the gravitational field in black hole/black brane spacetimes with anti-de Sitter asymptotics should exhibit similar scaling relatio… Show more

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Cited by 20 publications
(50 citation statements)
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“…This includes the use of a random external force to generate the turbulent flow, as well as considerations specific to simulating either a conformal fluid or an incompressible Navier-Stokes fluid. The equivalence between previously known results and the incompressible limit of the scaling relations derived in [1] is explicitly demonstrated. We give our results in section 4, where our numerical measurements of the scaling relations derived in [1] are presented.…”
Section: Jhep08(2017)027supporting
confidence: 58%
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“…This includes the use of a random external force to generate the turbulent flow, as well as considerations specific to simulating either a conformal fluid or an incompressible Navier-Stokes fluid. The equivalence between previously known results and the incompressible limit of the scaling relations derived in [1] is explicitly demonstrated. We give our results in section 4, where our numerical measurements of the scaling relations derived in [1] are presented.…”
Section: Jhep08(2017)027supporting
confidence: 58%
“…There has been some work on the analytical front [1,22,23] and several numerical investigations [1,13,[24][25][26][27][28][29][30][31]. Because correlation functions can indeed be measured in relevant scenarios -perhaps even in QG plasma [8,9,[32][33][34] -and interesting implications for the gravitational field follow from holography, it is of interest to further investigate relativistic turbulence.…”
Section: Jhep08(2017)027mentioning
confidence: 99%
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“…A recent review which examines both hydrodynamic and magnetohydrodynamic implementations of supersonic compressible turbulence on statistical quantities can be found in Falceta-Goncalves et al (2014). In this work, we follow the vast majority of investigations (Kuznetsov and Sereshchenko, 2015;Shivamoggi, 2015;Domaradzki and Carati, 2007;Sun, 2016;Westernacher-Schneider et al, 2015;Ottaviani, 1992;Qiu et al, 2016;Bershadskii, 2016) by utilizing the phenomenological description of turbulence 15 in Fourier space as well as the utilization of two-point velocity structure functions for the statistical examination of our high fidelity numerical simulations. In terms of reference scaling behavior, we shall be comparing our numerical results against the theories advanced in Shivamoggi (1992) under the assumption of isentropic flow.…”
Section: Introductionmentioning
confidence: 99%