For a quantum-corrected Schwarzschild black hole in a Kiselev perfect fluid, first-order PV criticality appears when the fluid parameter satisfies omega > -1/3 and omega differs from zero, while a Hawking-Page-like transition appears for omega = -1, with heat engine efficiencies depending on the…
Massive gravity with Lorentz symmetry breaking: black holes as heat engines
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
In extended phase space, a static black hole in massive gravity is studied as a holographic heat engine. In the massive gravity theory considered, the graviton gain a mass due to Lorentz symmetry breaking. Exact efficiency formula is obtained for a rectangle engine cycle for the black hole considered. The efficiency is computed by varying two parameters in the theory, the scalar charge Q and $\lambda$. The efficiency is compared with the Carnot efficiency for the heat engine. It is observed that when Q and $\lambda$ are increased that the efficiency for the rectangle cycle increases. When compared to the Schwarzschild AdS black hole, the efficiency for the rectangle cycle is larger for the Massive gravity black hole.
fields
gr-qc 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Effects of quantum corrections on the criticality and efficiency of black holes surrounded by a perfect fluid
For a quantum-corrected Schwarzschild black hole in a Kiselev perfect fluid, first-order PV criticality appears when the fluid parameter satisfies omega > -1/3 and omega differs from zero, while a Hawking-Page-like transition appears for omega = -1, with heat engine efficiencies depending on the…