Charged Embedded Horizons and their Area Evolution

The Embedded Horizon is defined to be a horizon that is in equilibrium with the exterior of the black hole, that is, isolated on the outside, but dynamically evolving on the inside, analogous to the inner and outer event horizons of the Reissner-Nordstrom black hole. This is shown as the result of charge variance on the horizon, which is expressed in electrical angular coordinates. The mass and energy of the black hole are discussed. The intrinsic metric is calculated by taking the electric potential into consideration. An area law evolution law is formulated, which suggests that the inner dynamical horizon evolves until it reaches the radius of the isolated horizon. The dynamical horizon, then, reaches equilibrium with the exterior, turning into an isolated horizon, thus turning extremal.