Thermodynamics of Plasmaballs and Plasmarings in 3+1 Dimensions
Shanthanu Bhardwaj, Jyotirmoy Bhattacharya
TL;DR
This work uses the AdS/CFT correspondence to study rotating, localized plasma configurations in 3+1 dimensions arising from Scherk-Schwarz compactification, predicting the thermodynamics of localized black holes and black rings in Scherk-Schwarz AdS_6. It derives an exact relativistic Navier–Stokes solution in the thin-ring limit, complemented by a thorough numerical analysis that maps the full thermodynamic phase space. The study confirms ball and ring (including pinched-ball) as the stationary rotating fluid solutions and reveals a continuous ball→pinched-ball→thin-ring transition, with the thin ring dominating the entropy at large angular momentum, and contrasts these results with conjectured flat-space phase diagrams. The results illuminate how AdS curvature and SS compactification qualitatively alter horizon topology phases and offer a controlled framework for investigating stability and dynamics of higher-dimensional black holes and rings via boundary fluid dynamics.
Abstract
We study localized plasma configurations in 3+1 dimensional massive field theories obtained by Scherk-Schwarz compactification of 4+1 dimensional CFT to predict the thermodynamic properties of localized blackholes and blackrings in Scherk-Schwarz compactified $AdS_6$ using the AdS/CFT correspondence. We present an exact solution to the relativistic Navier-Stokes equation in the thin ring limit of the fluid configuration. We also perform a thorough numerical analysis to obtain the thermodynamic properties of the most general solution. Finally we compare our results with the recent proposal for the phase diagram of blackholes in six flat dimensions and find some similarities but other differences.
