2019
DOI: 10.1103/physrevd.100.084061
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Charged accelerating black hole in f(R) gravity

Abstract: We obtain a charged accelerating AdS black hole solution in f (R) gravity and investigate its thermodynamic behaviour. We consider low-acceleration black holes that do not have an acceleration horizon and obtain the first law of thermodynamics for them. We further study the parameter space of charged slowly accelerating f (R) AdS black holes before investigating the behaviour of the free energy in both the canonical and grand canonical ensembles. We find a generalization of the reverse isoperimetric inequality… Show more

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Cited by 32 publications
(21 citation statements)
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References 88 publications
(129 reference statements)
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“…However, in an inhomogeneous plasma, these results are only directly applicable to instabilities that saturate convectively (i.e., undergo finite spatial amplification) because the convective gain is directly related to the linear growth rate. Two-plasmon decay becomes absolutely unstable (temporal growth at a fixed point in space) when the convective gain is relatively small ( 2π) [31]. The linear growth rate plays a reduced role in absolute instabilities because they always grow until saturated by some nonlinear mechanism.…”
mentioning
confidence: 99%
“…However, in an inhomogeneous plasma, these results are only directly applicable to instabilities that saturate convectively (i.e., undergo finite spatial amplification) because the convective gain is directly related to the linear growth rate. Two-plasmon decay becomes absolutely unstable (temporal growth at a fixed point in space) when the convective gain is relatively small ( 2π) [31]. The linear growth rate plays a reduced role in absolute instabilities because they always grow until saturated by some nonlinear mechanism.…”
mentioning
confidence: 99%
“…To start, one reconsiders the study of the physical content of f ðRÞ gravity. According to [53], its action containing a Maxwell gauge term takes the following general form…”
Section: Charged Accelerating Fðrþ Black Hole Backgroundmentioning
confidence: 99%
“…Since the paths in Eq. (18) contain many segments, we consider interleaving these segments with a dynamical decoupling sequence [28]. Consider a three-level system experiencing decay, induced by the system-environment interaction Hamiltonian…”
Section: B Dynamical Decouplingmentioning
confidence: 99%