activity
20022009
most citedNonlinear Fluid Dynamics from Gravity

1.2k citations · 2.7k across the 12 of their papers we have counts for

collaborators

21 papers

hep-th2009176 cited

Weak Field Black Hole Formation in Asymptotically AdS Spacetimes

Sayantani Bhattacharyya, Shiraz Minwalla

We use the AdS/CFT correspondence to study the thermalization of a strongly coupled conformal field theory that is forced out of its vacuum by a source that couples to a marginal o…

hep-th2008122 cited

The Incompressible Non-Relativistic Navier-Stokes Equation from Gravity

Sayantani Bhattacharyya, Shiraz Minwalla, Spenta R. Wadia

We note that the equations of relativistic hydrodynamics reduce to the incompressible Navier-Stokes equations in a particular scaling limit. In this limit boundary metric fluctuati…

hep-th2008154 cited

Conformal Nonlinear Fluid Dynamics from Gravity in Arbitrary Dimensions

Sayantani Bhattacharyya, R. Loganayagam, Ipsita Mandal +2

We generalize recent work to construct a map from the conformal Navier Stokes equations with holographically determined transport coefficients, in d spacetime dimensions, to the se…

hep-th2008176 cited

Superconformal Indices for Chern Simons Theories

Jyotirmoy Bhattacharya, Shiraz Minwalla

Aharony, Bergman, Jafferis and Maldacena have recently proposed a dual gravitational description for a family of superconformal Chern Simons theories in three spacetime dimensions.…

hep-th2008233 cited

Local Fluid Dynamical Entropy from Gravity

Sayantani Bhattacharyya, Veronika E Hubeny, R. Loganayagam +5

Spacetime geometries dual to arbitrary fluid flows in strongly coupled N=4 super Yang Mills theory have recently been constructed perturbatively in the long wavelength limit. We de…

hep-th200881 cited

Comments on 1/16 BPS Quantum States and Classical Configurations

Lars Grant, Pietro A. Grassi, Seok Kim +1

We formulate the problem of counting 1/16 BPS states of N = 4 Yang Mills theory as the enumeration of the local cohomology of an operator acting on holomorphic fields on C^2. We st…