The inverse mean curvature flow in cosmological spacetimes
Gerhardt, Claus
Adv. Theor. Math. Phys., Tome 12 (2008) no. 3, p. 1183-1207 / Harvested from Project Euclid
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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.
Publié le : 2008-12-15
Classification:  
@article{1221834531,
     author = {Gerhardt, Claus},
     title = {The inverse mean curvature flow in cosmological spacetimes},
     journal = {Adv. Theor. Math. Phys.},
     volume = {12},
     number = {3},
     year = {2008},
     pages = { 1183-1207},
     language = {en},
     url = {http://dml.mathdoc.fr/item/1221834531}
}

Gerhardt, Claus. The inverse mean curvature flow in cosmological spacetimes. Adv. Theor. Math. Phys., Tome 12 (2008) no. 3, pp.  1183-1207. http://gdmltest.u-ga.fr/item/1221834531/