Black hole Area-Angular Momentum-Charge inequality in dynamical non-vacuum spacetimes.

MARÍA EUGENIA GABACH CLEMENT; JOSE LUIS JARAMILLO

PHYSICAL REVIEW D

AMER PHYSICAL SOC

Año: 2012

1550-7998

We show that the area-angular momentum-charge inequality (A/(4pi))^2 geq (2J)^2 + (Q_E^2 + Q_M^2)^2 holds for apparent horizons of electrically and magnetically charged rotating black holes in generic dynamical and non-vacuum spacetimes. More specifically, this quasi-local inequality applies to axially symmetric closed outermost stably marginally (outer) trapped surfaces, embedded in non-necessarily axisymmetric black hole spacetimes with non-negative cosmological constant and matter content satisfying the dominant energy condition.