Some remarks on the size of bodies and black holes
Gregory J. Galloway, Niall O'Murchadha

TL;DR
This paper explores how stable marginally outer trapped surfaces can be used to analyze the size of material bodies and black holes, extending previous results to more general initial data sets.
Contribution
It generalizes earlier findings by applying stable marginally outer trapped surfaces to broader initial data configurations beyond maximal or time-symmetric cases.
Findings
Extended size and area bounds to general initial data sets
Applied trapped surface techniques to material bodies and black holes
Broadened the scope of previous geometric inequalities
Abstract
We consider the application of stable marginally outer trapped surfaces to problems concerning the size of material bodies and the area of black holes. The results presented extend to general initial data sets (V,g,K) previous results assuming either maximal (tr K = 0) or time-symmetric (K = 0) initial data.
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