Abstract:Let (M n , g) be an n-dimensional compact connected Riemannian manifold with smooth boundary. We show that the presence of a nontrivial conformal gradient vector field on M , with an appropriate control on the Ricci curvature, causes M to be isometric to a hemisphere of S n . We also prove that if an Einstein manifold with boundary admits nonzero conformal gradient vector field, then its scalar curvature is positive and it is isometric to a hemisphere of S n . Furthermore, we prove that if M admits a nontrivia… Show more
“…Moreover, the second and third authors obtained integral expressions involving the conformal field and the conformal factor (see [13], Lemmas 2.1 and 2.4). More precisely, they proved Lemma 2.…”
Section: Preliminariesmentioning
confidence: 99%
“…An interesting problem in Riemannian geometry is to find characterizations of spheres and hemispheres in the class of compact connected Riemannian manifolds with empty and non-empty boundary, respectively (see, e.g., [1,8,9,10,23,13,19,20]).…”
Let (M n , g) be an n-dimensional compact connected Riemannian manifold with smooth boundary. In this article, we study the effects of the presence of a nontrivial conformal vector field on (M n , g). We used the wellknown de-Rham Laplace operator and a nontrivial solution of the famous Fischer-Marsden differential equation to provide two characterizations of the hemisphere S n + (c) of constant curvature c > 0. As a consequence of the characterization using the Fischer-Marsden equation, we prove the cosmic no-hair conjecture under a given integral condition.
“…Moreover, the second and third authors obtained integral expressions involving the conformal field and the conformal factor (see [13], Lemmas 2.1 and 2.4). More precisely, they proved Lemma 2.…”
Section: Preliminariesmentioning
confidence: 99%
“…An interesting problem in Riemannian geometry is to find characterizations of spheres and hemispheres in the class of compact connected Riemannian manifolds with empty and non-empty boundary, respectively (see, e.g., [1,8,9,10,23,13,19,20]).…”
Let (M n , g) be an n-dimensional compact connected Riemannian manifold with smooth boundary. In this article, we study the effects of the presence of a nontrivial conformal vector field on (M n , g). We used the wellknown de-Rham Laplace operator and a nontrivial solution of the famous Fischer-Marsden differential equation to provide two characterizations of the hemisphere S n + (c) of constant curvature c > 0. As a consequence of the characterization using the Fischer-Marsden equation, we prove the cosmic no-hair conjecture under a given integral condition.
“…Then, they used that expression to obtain a Minkowski type integral formula for compact Riemannian and spacelike hypersurfaces, and applied this to deduce some interesting results concerning the characterization of compact Riemannian and spacelike hypersurfaces under certain hypotheses such as the constancy of the mean curvature or the assumption that the ambient space is Einstein or a product space. For more recent references pertaining to this work, we may cite [18][19][20][21].…”
We obtain some generalized Minkowski type integral formulas for compact Riemannian (resp., spacelike) hypersurfaces in Riemannian (resp., Lorentzian) manifolds in the presence of an arbitrary vector field that we assume to be timelike in the case where the ambient space is Lorentzian. Some of these formulas generalize existing formulas in the case of conformal and Killing vector fields. We apply these integral formulas to obtain interesting results concerning the characterization of such hypersurfaces in some particular cases such as when the ambient space is Einstein admitting an arbitrary (in particular, conformal or Killing) vector field, and when the hypersurface has a constant mean curvature.
“…Conformal vector fields and conformal mappings play important roles in the geometry of (pseudo-)Riemannian manifolds as well as in the general relativity (see, e.g., [1][2][3][4][5]). The characterization of important spaces, such as Euclidean spaces, Euclidean spheres and hyperbolic spaces, represents one of the most fascinating problems in Riemannian geometry.…”
Section: Introductionmentioning
confidence: 99%
“…and using Equations ( 4) and ( 5), we see that the function f on the sphere S m (c) satisfies the Fischer-Marsden Equation (2). Recall that a smooth vector field u on a Riemannian manifold (M, g) is said to be a conformal vector field, if…”
We study the effect of a nontrivial conformal vector field on the geometry of compact Riemannian spaces. We find two new characterizations of the m-dimensional sphere Sm(c) of constant curvature c. The first characterization uses the well known de-Rham Laplace operator, while the second uses a nontrivial solution of the famous Fischer–Marsden differential equation.
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