Abstract
Abstract
Given spherically symmetric characteristic initial data for the Einstein-scalar field system with a positive cosmological constant, we provide a criterion, in terms of the dimensionless size and dimensionless renormalized mass content of an annular region of the data, for the formation of a future trapped surface. This corresponds to an extension of Christodoulou’s classical criterion by the inclusion of the cosmological term.
Funder
CERN
Fundação para a Ciência e a Tecnologia
Subject
Physics and Astronomy (miscellaneous)
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