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2011

Phenomenology of Irreversible Processes from Gravity

Iyer, Ramakrishnan, Mukhopadhyay, Ayan

Understand

We propose that the space-time evolution of strongly coupled matter formed by ultra-relativistic heavy ion collisions can be modelled by phenomenological equations involving the energy-momentum tensor and conserved currents alone.

These equations can describe the late stage of local chemical and thermal equilibration of the matter formed after collisions, and its subsequent transition to hydrodynamic expansion in an unified framework.
The full set of equations include local energy, momentum and charge conservation; but also additional equations for evolution of non-equilibrium variables.
These equations with precisely determined phenomenological parameters can be obtained by the AdS/CFT correspondence.