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Polyharmonic hypersurfaces into pseudo-Riemannian space forms

In this paper, we shall assume that the ambient manifold is a pseudo-Riemannian space form [Formula: see text] of dimension [Formula: see text] and index t ([Formula: see text] and [Formula: see text] ). We shall study hypersurfaces [Formula: see text] which are polyharmonic of order r (briefly, r-h...

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Detalles Bibliográficos
Autores principales: Branding, V., Montaldo, S., Oniciuc, C., Ratto, A.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9950211/
https://www.ncbi.nlm.nih.gov/pubmed/36852229
http://dx.doi.org/10.1007/s10231-022-01263-1
Descripción
Sumario:In this paper, we shall assume that the ambient manifold is a pseudo-Riemannian space form [Formula: see text] of dimension [Formula: see text] and index t ([Formula: see text] and [Formula: see text] ). We shall study hypersurfaces [Formula: see text] which are polyharmonic of order r (briefly, r-harmonic), where [Formula: see text] and either [Formula: see text] or [Formula: see text] . Let A denote the shape operator of [Formula: see text] . Under the assumptions that [Formula: see text] is CMC and [Formula: see text] is a constant, we shall obtain the general condition which determines that [Formula: see text] is r-harmonic. As a first application, we shall deduce the existence of several new families of proper r-harmonic hypersurfaces with diagonalizable shape operator, and we shall also obtain some results in the direction that our examples are the only possible ones provided that certain assumptions on the principal curvatures hold. Next, we focus on the study of isoparametric hypersurfaces whose shape operator is non-diagonalizable and also in this context we shall prove the existence of some new examples of proper r-harmonic hypersurfaces ([Formula: see text] ). Finally, we shall obtain the complete classification of proper r-harmonic isoparametric pseudo-Riemannian surfaces into a three-dimensional Lorentz space form.