We present a type-IIB supergravity solution dual to a spatially anisotropic finite-temperature N = 4 super-Yang-Mills plasma. The solution is static and completely regular. The full geometry can be viewed as a renormalization group flow from an ultraviolet anti-de Sitter geometry to an infrared Lifshitz-like geometry. The anisotropy can be equivalently understood as resulting from a position-dependent θ term or from a nonzero number density of dissolved D 7 -branes. The holographic stress tensor is conserved and anisotropic. The presence of a conformal anomaly plays an important role in the thermodynamics. The phase diagram exhibits homogeneous and inhomogeneous (i.e., mixed) phases. In some regions the homogeneous phase displays instabilit...
Abstract A relativistic fluid in 3+1 dimensions with a global U(1) symmetry admits nine independent ...
Abstract We use holography to investigate the process of homogeneous isotropization and thermalizati...
We study the energy loss of a quark moving in the strongly coupled $\mathcal{N} = 4$ supersymmetric ...
We present a type-IIB supergravity solution dual to a spatially anisotropic finite-temperature N = 4...
We present a IIB supergravity solution dual to a spatially anisotropic finite-temperature N=4 super ...
We present a IIB supergravity solution dual to a spatially anisotropic finite-temperature N=4 super ...
We extend our analysis of a IIB supergravity solution dual to a spatially anisotropic finite-tempera...
We extend our analysis of a IIB supergravity solution dual to a spatially anisotropic finite-tempera...
We extend our analysis of a IIB supergravity solution dual to a spatially anisotropic finite-tempera...
We present a type-IIB supergravity solution dual to a spatially anisotropic finite-temperature N = 4...
Generically, the black brane solution with planar horizons is thermodynamically stable. We find a co...
We present a type IIB supergravity solution dual to a spatially anisotropic N $$ \mathcal{N} $$ =4 s...
AbstractGenerically, the black brane solution with planar horizons is thermodynamically stable. We f...
Black hole solutions of type IIB supergravity have been previously constructed that describe the N=4...
Black hole solutions of type IIB supergravity have been previously constructed that describe the N=4...
Abstract A relativistic fluid in 3+1 dimensions with a global U(1) symmetry admits nine independent ...
Abstract We use holography to investigate the process of homogeneous isotropization and thermalizati...
We study the energy loss of a quark moving in the strongly coupled $\mathcal{N} = 4$ supersymmetric ...
We present a type-IIB supergravity solution dual to a spatially anisotropic finite-temperature N = 4...
We present a IIB supergravity solution dual to a spatially anisotropic finite-temperature N=4 super ...
We present a IIB supergravity solution dual to a spatially anisotropic finite-temperature N=4 super ...
We extend our analysis of a IIB supergravity solution dual to a spatially anisotropic finite-tempera...
We extend our analysis of a IIB supergravity solution dual to a spatially anisotropic finite-tempera...
We extend our analysis of a IIB supergravity solution dual to a spatially anisotropic finite-tempera...
We present a type-IIB supergravity solution dual to a spatially anisotropic finite-temperature N = 4...
Generically, the black brane solution with planar horizons is thermodynamically stable. We find a co...
We present a type IIB supergravity solution dual to a spatially anisotropic N $$ \mathcal{N} $$ =4 s...
AbstractGenerically, the black brane solution with planar horizons is thermodynamically stable. We f...
Black hole solutions of type IIB supergravity have been previously constructed that describe the N=4...
Black hole solutions of type IIB supergravity have been previously constructed that describe the N=4...
Abstract A relativistic fluid in 3+1 dimensions with a global U(1) symmetry admits nine independent ...
Abstract We use holography to investigate the process of homogeneous isotropization and thermalizati...
We study the energy loss of a quark moving in the strongly coupled $\mathcal{N} = 4$ supersymmetric ...