Phase transitions of black strings in dynamical Chern-Simons modified gravity

We study conserved charges and thermodynamics of analytic rotating anti-de Sitter black holes with extended horizon topology-also known as black strings-in dynamical Chern-Simons modified gravity. The solution is supported by a scalar field with an axionic profile that depends linearly on the coordinate that spans the string. We compute conserved charges by making use of the renormalized boundary stress energy tensor. Then, by adopting the Noether-Wald formalism, we compute the black string entropy and obtain its area law. Indeed, the reduced Euclidean Hamiltonian approach shows that these methods yield a consistent first law of thermodynamics. Additionally, we derive a Smarr formula using a radial conservation law associated to the scale invariance of the reduced action and obtain a Cardy formula for the black string. A first-order phase transition takes place at a critical temperature between the ground state and the black string, above which the black string is the thermodynamically favored configuration.

Automated summary

We study conserved charges and thermodynamics of analytic rotating anti-de Sitter black holes with extended horizon topology. We compute conserved charges using the renormalized boundary stress energy tensor and calculate the black hole entropy. We also derive a Smarr formula and a Cardy formula.