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A note on inverse mean curvature flow in cosmological spacetimes
Authors:Heiko Kröner
Affiliation:Mathematisches Institut, Universit?t Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
Abstract:In 12 Gerhardt proves longtime existence for the inverse mean curvature flow in globally hyperbolic Lorentzian manifolds with compact Cauchy hypersurface, which satisfy three main structural assumptions: a strong volume decay condition, a mean curvature barrier condition and the timelike convergence condition. Furthermore, it is shown in 12 that the leaves of the inverse mean curvature flow provide a foliation of the future of the initial hypersurface.We show that this result persists, if we generalize the setting by leaving the mean curvature barrier assumption out. For initial hypersurfaces with sufficiently large mean curvature we can weaken the timelike convergence condition to a physically relevant energy condition.
Keywords:Lorentzian manifold  cosmological spacetime  general relativity  inverse mean curvature flow  35J60  53C21  53C44  53C50  58J05
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