New area bounds for marginally trapped surfaces are derived from Einstein tensor components and stability parameters, realized in ultra-massive spacetimes even for non-positive cosmological constant under strong energy-momentum conditions.
Quantum Grav.24(2007) 3091–3124 13
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New bounds for the area of MOTS and generalized ultra-massive spacetimes
New area bounds for marginally trapped surfaces are derived from Einstein tensor components and stability parameters, realized in ultra-massive spacetimes even for non-positive cosmological constant under strong energy-momentum conditions.