Complexity of the Einstein-Born-Infeld-Massive Black holes
arXiv:1810.04792
Abstract
Motivated by interesting correspondence between computational complexity in a CFT and the action evaluated on a WDW patch in the bulk, we study the complexity of the Einstein-massive black holes in the presence of BI nonlinear electrodynamics. The upper limit of Llyod bound according to the WDW patch is investigated and it is proved that Llyod bound is held.
arXiv comment11 pages
References in corpus (24)
- Resummation of Massive Gravity
- Generalization of the Fierz-Pauli Action
- Ultimate physical limits to computation
- Theoretical Aspects of Massive Gravity
- The Stretched Horizon and Black Hole Complementarity
- Resolving the Ghost Problem in non-Linear Massive Gravity
- Complexity and Shock Wave Geometries
- Quantum Computation as Geometry
- On Non-Linear Actions for Massive Gravity
- Gravitational action with null boundaries
- Thermodynamics of Black Holes in Massive Gravity
- Complexity Growth for AdS Black Holes
- Einstein-Born-Infeld-Massive Gravity: adS-Black Hole Solutions and their Thermodynamical properties
- Quantum Complexity and Negative Curvature
- Topological charged black holes in massive gravity's rainbow and their thermodynamical analysis through various approaches
- Aspects of Born-Infeld Theory and String/M-Theory
- The Melvin Universe in Born-Infeld Theory and other Theories of Non-Linear Electrodynamics
- New perspective for black hole thermodynamics in Gauss-Bonnet-Born-Infeld massive gravity
- Charged BTZ black holes in the context of massive gravity's rainbow
- The effect of Dilaton on the holographic complexity growth
- Action growth of charged black holes with a single horizon
- Complexity growth rates for AdS black holes in massive gravity and gravity
- Phase transition of charged black holes in massive gravity through new methods
- Three dimensional magnetic solutions in massive gravity with (non)linear field