The inverse mean curvature flow in cosmological spacetimes
Source: Adv. Theor. Math. Phys.
Volume 12, Number 6
We prove that the leaves of an inverse mean curvature flow provide a foliation of a future end of a cosmological spacetime $N$ under the necessary and sufficient assumptions that $N$ satisfies a future mean curvature barrier condition and a strong volume decay condition. Moreover, the flow parameter t can be used to define a new physically important time function.
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Links and Identifiers
Permanent link to this document: http://projecteuclid.org/euclid.atmp/1221834531
Mathematical Reviews number (MathSciNet): MR2443263
Zentralblatt MATH identifier: 1153.83016