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We prove that a spacelike spherical symmetric constant mean curvature (SSCMC) surface and a general spacelike constant mean curvature (CMC) surface with certain boundary condition at the future null-infinity in Schwarzschild spacetime are…

Differential Geometry · Mathematics 2022-02-03 Caiyan Li , Yuguang Shi , Luen-Fai Tam

We solve spacelike spherically symmetric constant mean curvature (SS-CMC) hypersurfaces in Schwarzschild spacetimes and analyze their asymptotic behavior near the coordinate singularity r = 2M. Furthermore, we join SS-CMC hypersurfaces in…

Differential Geometry · Mathematics 2011-12-08 Kuo-Wei Lee , Yng-Ing Lee

The problem of existence of spacelike hypersurfaces with constant mean curvature in asymptotically flat spacetimes is considered for a class of asymptotically Schwarzschild spacetimes satisfying an interior condition. Using a barrier…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Lars Andersson , Mirta S. Iriondo

The spherically symmetric null hypersurfaces in a Schwarzschild spacetime are smooth away from the singularities and foliate the spacetime. We prove the existence of more general foliations by null hypersurfaces without the spherical…

Differential Geometry · Mathematics 2022-07-12 Pengyu Le

We first summarize the characterization of smooth spacelike spherically symmetric constant mean curvature (SS-CMC) hypersurfaces in the Schwarzschild spacetime and Kruskal extension. Then use the characterization to prove special SS-CMC…

Differential Geometry · Mathematics 2016-05-25 Kuo-Wei Lee , Yng-Ing Lee

We consider complete spacelike hypersurfaces with constant mean curvature in the open region of de Sitter space known as the steady state space. We prove that if the hypersurface is bounded away from the infinity of the ambient space, then…

Differential Geometry · Mathematics 2009-02-17 Alma L. Albujer , Luis J. Alias

For asymptotically flat spacetimes, using the inverse mean curvature flow, we show that any compact $2$-surface, $S_0$, whose mean curvature and its derivative for outward direction are positive in spacelike hypersurface with non-negative…

General Relativity and Quantum Cosmology · Physics 2017-04-19 Tetsuya Shiromizu , Yoshimune Tomikawa , Keisuke Izumi , Hirotaka Yoshino

We establish a new CMC (constant mean curvature) existence result for cosmological spacetimes, i.e., globally hyperbolic spacetimes with compact Cauchy surfaces satisfying the strong energy condition. If the spacetime contains an expanding…

Differential Geometry · Mathematics 2026-02-17 Gregory J. Galloway , Eric Ling

Recently, there have been efforts to solve Einstein's equation in the context of a conformal compactification of space-time. Of particular importance in this regard are the so called CMC-foliations, characterized by spatial hyperboloidal…

General Relativity and Quantum Cosmology · Physics 2014-04-14 David Schinkel , Rodrigo Panosso Macedo , Marcus Ansorg

We consider a family of spherical three dimensional spacelike slices embedded in the Schwarzschild solution. The mean curvature is constant on each slice but can change from slice to slice. We give a simple expression for an everywhere…

General Relativity and Quantum Cosmology · Physics 2009-09-02 Edward Malec , Niall O'Murchadha

We construct a $T$-axisymmetric, spacelike, spherically symmetric, constant mean curvature hypersurfaces foliation in the Kruskal extension with properties that the mean curvature varies in each slice and ranges from minus infinity to plus…

Differential Geometry · Mathematics 2016-11-02 Kuo-Wei Lee

We prove two rigidity results for surfaces lying in the standard null hypersurfaces of Schwarzschild spacetime satisfying certain mean curvature type equations. The first is for the equation $\alpha_H = - d\log |H|$ studied in \cite{WWZ}.…

Differential Geometry · Mathematics 2023-06-14 Po-Ning Chen , Ye-Kai Wang

Conformal mappings of surfaces of constant mean curvature onto compact bounded background spaces are constructed for Minkowski space-time and for Schwarzschild black hole spacetimes. In the black hole example, it is found that initial data…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Robert H. Gowdy

We consider spacelike graphs $\Gamma_f$ of simple products $(M\times N, g\times -h)$ where $(M,g)$ and $(N,h)$ are Riemannian manifolds and $f:M\to N$ is a smooth map. Under the condition of the Cheeger constant of $M$ to be zero and some…

Differential Geometry · Mathematics 2007-05-23 Isabel M. C. Salavessa

Spacelike surfaces in the Lorentz-Minkowski space L^3 can be endowed with two different Riemannian metrics, the metric inherited from L^3 and the one induced by the Euclidean metric of R^3. It is well known that the only surfaces with zero…

Differential Geometry · Mathematics 2016-04-15 Alma L. Albujer , Magdalena Caballero

The constant mass function foliation has been shown useful for studying the null Penrose inequality on a null hypersurface, because of the monotonicity formula of Hawking mass along such a foliation. In this paper, we show the global…

Differential Geometry · Mathematics 2024-04-29 Pengyu Le

We examine the geometry of a generalized uncertainty-inspired quantum black hole. The diagonal line element is not $t$-$r$ symmetric, i.e. $g_{00} \ne -1/g_{11}$, which leads to an interesting approach to resolving the classical curvature…

General Relativity and Quantum Cosmology · Physics 2025-04-24 Douglas M. Gingrich , Saeed Rastgoo

We study singularities of spacelike, constant (non-zero) mean curvature (CMC) surfaces in the Lorentz-Minkowski 3-space $L^3$. We show how to solve the singular Bj\"orling problem for such surfaces, which is stated as follows: given a real…

Differential Geometry · Mathematics 2011-04-01 David Brander

Uniqueness and non-existence results on complete constant mean curvature spacelike hypersurfaces lying between two spacelike slice in the Einstein-de Sitter spacetime are given. They are obtained from a Liouvielle-type theorem applied to a…

Mathematical Physics · Physics 2014-01-06 Rafael M. Rubio

We consider space-times which are asymptotically flat at spacelike infinity, i^0. It is well known that, in general, one cannot have a smooth differentiable structure at i^0, but have to use direction dependent structures. Instead of the…

General Relativity and Quantum Cosmology · Physics 2009-10-30 Magnus Herberthson
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