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Similar

J. Vredevoogd and S. Pratt, “Universal flow in the first stage of relativistic heavy ion collisions,” Phys.Rev
Original
2009
Cited alongside, same era.
P. M. Chesler and L. G. Yaffe, “Boost invariant flow, black hole formation, and far-from-equilibrium dynamics in 𝒩 = 4 \mathcal{N}=4 supersymmetric Yang-Mills theory,” Phys.Rev
Original
2010
Cited alongside, same era.
P. M. Chesler and L. G. Yaffe, “Holography and colliding gravitational shock waves in asymptotically AdS 5 spacetime,” Phys.Rev.Lett
Original
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Cited alongside, same era.
H. Bantilan, F. Pretorius, and S. S. Gubser, “Simulation of asymptotically AdS 5 spacetimes with a generalized harmonic evolution scheme,” Phys.Rev
Original
2012
Cited alongside, same era.
M. P. Heller, D. Mateos, W. van der Schee, and D. Trancanelli, “Strong coupling isotropization of non-Abelian plasmas simplified,” Phys.Rev.Lett

Then

W. van der Schee, P. Romatschke, and S. Pratt, “Fully dynamical simulation of central nuclear collisions,” Phys.Rev.Lett
Original
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Later among the works it cites.
M. P. Heller, D. Mateos, W. van der Schee, and M. Triana, “Holographic isotropization linearized,” JHEP
Original
2013
Later among the works it cites.
P. M. Chesler and L. G. Yaffe, “Numerical solution of gravitational dynamics in asymptotically anti-de Sitter spacetimes,” JHEP
Original
2014
Later among the works it cites.
M. Luzum and H. Petersen, “Initial state fluctuations and final state correlations in relativistic heavy-ion collisions,” J.Phys
Original
2014
Later among the works it cites.
S. Floerchinger and U. A. Wiedemann, “Statistics of initial density perturbations in heavy ion collisions and their fluid dynamic response,” JHEP

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2015

Holography and off-center collisions of localized shock waves

Chesler, Paul M., Yaffe, Laurence G.

Understand

Using numerical holography, we study the collision, at non-zero impact parameter, of bounded, localized distributions of energy density chosen to mimic relativistic heavy ion collisions, in strongly coupled N = 4 supersymmetric Yang-Mills theory.

Both longitudinal and transverse dynamics in the dual field theory are properly described.
Using the gravitational description we solve 5D Einstein equations, without dimensionality reducing symmetry restrictions, to find the asymptotically anti-de Sitter spacetime geometry.
Implications of our results on the understanding of early stages of heavy ion collisions, including the development of transverse radial flow, are discussed.