Allan Adams, Tarek Anous, Jaehoon Lee, Sho Yaida


arXiv:1406.1498



Supercooled liquids exhibit a dramatic dynamical slowdown as the temperature is lowered. This can be attributed to relaxation proceeding via large structural rearrangements, whose characteristic size increases as the temperature decreases. These cooperative rearrangements are well modeled by instantons in a replica effective field theory, with the size of the dominant instanton encoding the liquid's cavity point-to-set correlation length. We show that, for a wide range of parameters, a novel class of replica-symmetry-breaking instantons dominates. We systematically construct these instantons and explore the subtle energetics governing their existence. Our methods extend naturally to the full parameter space of the effective theory, laying the groundwork for a complete analysis of point-to-set correlations in glassy systems.

 


Allan Adams, Paul Chesler and Hong Liu


arXiv:1307.7267,  PRL 112 (2014) 151602



Holography relates fluid flows in “normal” quantum liquids (vs. “superfluids”) to the evolving geometry of dynamical black holes.  We use this duality to study turbulence in quantum liquids by numerically solving the Einstein equations governing the dual black hole spacetimes. For 2+1 dimensional liquids, both bulk geometry and the dual liquid display signatures of an inverse cascade.  Numerical and analytic arguments demonstrate that black holes dual to d-dimensional turbulent flows have horizons with fractal structures of fractal dimension D=d+4/3.


 


Allan Adams, Paul Chesler and Hong Liu


arXiv:1212.0281,  Science 341 (6144) 368-372




Turbulence provides a fascinating window into superfluid dynamics. Since vortices are central to the turbulent state, understanding quantum turbulence requires control over not just the hydrodynamics but also the quantum structure of vortex cores.  We study a holographic version of this problem, where the quantum dynamics are encoded in a classical effective action in an emergent spacetime.  We find that decaying turbulent flows in  holographic superfluids exhibit approximate Kolmogorov scaling and a clear direct cascade.

 


Allan Adams, Nathan Benjamin, Arvin Moghaddam , Wociech Musial


arXiv:1411.2001



Building dynamical black holes spacetimes requires solving the fully 4-dimensional Einstein equations, a highly-nonlinear set of partial differential equations which govern the time-evolution of spacetime.  For asymptotically-AdS spacetimes, holography reduces the problem to the numerical solution of 3-dimensional hydrodynamics.  By numerically solving 3-dimensional hydro and implementing the holographic map, one may numerically construct highly-accurate dynamical spacetimes without ever solving the 4-dimensional Einstein equations directly.