Black-hole dynamics in BHT massive gravity

Understand

Using an exact Vaidya-type null-dust solution, we study the area and entropy laws for dynamical black holes defined by a future outer trapping horizon in (2+1)-dimensional Bergshoeff-Hohm-Townsend (BHT) massive gravity.

• We consider the theory admitting a degenerate (anti-)de Sitter vacuum and pure BHT gravity.
• It is shown that, while the area of a black hole decreases by the injection of a null dust with positive energy density in several cases, the Wald-Kodama dynamical entropy always increases.