M. do Carmo
Instituto Nacional de Matemática Pura e Aplicada
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Transactions of the American Mathematical Society | 1983
M. do Carmo; Marcos Dajczer
Rotation hypersurfaces in spaces of constant curvature are defined and their principal curvatures are computed. A local characterization of such hypersurfaces, with dimensions greater than two, is given in terms of principal curvatures. Some special cases of rotation hypersurfaces, with constant mean curvature, in hyperbolic space are studied. In particular, it is shown that the well-known conjugation between the helicoid and the catenoid in euclidean three-space extends naturally to hyperbolic three-space H3 ; in the latter case, catenoids are of three different types and the explicit correspondence is given. It is also shown that there exists a family of simply-connected, complete, embedded, nontotally geodesic stable minimal surfaces in H3.
Annals of Global Analysis and Geometry | 2012
Pierre Bérard; M. do Carmo; W. Santos
The main result of this paper states that the traceless second fundamental tensor \({A}^{0}\)of an n-dimensional complete hypersurface M, with constant mean curvature H and finite total curvature, \(\int{M}^{|A^0|^n{d\nu}}{M} 0,\) any such surface must be compact.
Commentarii Mathematici Helvetici | 1986
M. do Carmo; J. de M. Gomes; G. Thorbergsson
This paper deals with complete, properly embedded hypersurfaces M n with constant mean curvature H of the hyperbolic space H n+1, and addresses itself to the following general question. How is the behaviour of such hypersurfaces influenced by their behaviour at infinity?
Commentarii Mathematici Helvetici | 2000
M. do Carmo; Manuel Ritoré; Antonio Ros
Abstract. Let Mn be a compact (two-sided) minimal hypersurface in a Riemannian manifold
Proceedings of the American Mathematical Society | 1972
M. do Carmo; B. Lawson
\bar M^{n+1}
Mathematische Zeitschrift | 1993
Hilário Alencar; M. do Carmo; A. G. Colares
. It is a simple fact that if
Mathematische Zeitschrift | 1997
Pierre Bérard; M. do Carmo; W. Santos
\bar M
Commentarii Mathematici Helvetici | 2002
Hilário Alencar; M. do Carmo; W. Santos
has positive Ricci curvature then M cannot be stable (i.e. its Jacobi operator L has index at least one). If
Archiv der Mathematik | 1993
Hilário Alencar; M. do Carmo
\bar M = S^{n+1}
Boletim Da Sociedade Brasileira De Matematica | 1971
M. do Carmo; Erica Souto Abreu Lima
is the unit sphere and L has index one, then it is known that M must be a totally geodesic equator.¶We prove that if