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Closed Biconservative Hypersurfaces in Spheres

Stefano Montaldo, Cezar Oniciuc, Alvaro Pampano

TL;DR

The paper addresses the existence and structure of non-CMC biconservative rotational hypersurfaces in space forms, focusing on compact examples in spheres. It proves that their profile curves are $p$-elastic with $p=\frac{n-2}{n+1}$ and develops a variational framework around $\mathbf{\Theta}_p(\gamma)=\int \kappa^p ds$. Using the Euler–Lagrange equation and a closure analysis, the authors establish a discrete biparametric family of closed, non-CMC rotational biconservative hypersurfaces in $\mathbb{S}^n(\rho)$ for every $n\ge3$, none embedding. The results generalize known 3D classifications to arbitrary dimension and provide explicit closure criteria via the phase-integral $I(d)$.

Abstract

We characterise the profile curves of non-CMC biconservative rotational hypersurfaces of space forms $N^n(ρ)$ as $p$-elastic curves, for a suitable rational number $p\in[1/4,1)$ which depends on the dimension $n$ of the ambient space. Analysing the closure conditions of these $p$-elastic curves, we prove the existence of a discrete biparametric family of non-CMC closed (i.e., compact without boundary) biconservative hypersurfaces in $\mathbb{S}^n(ρ)$. None of these hypersurfaces can be embedded in $\mathbb{S}^n(ρ)$.

Closed Biconservative Hypersurfaces in Spheres

TL;DR

The paper addresses the existence and structure of non-CMC biconservative rotational hypersurfaces in space forms, focusing on compact examples in spheres. It proves that their profile curves are -elastic with and develops a variational framework around . Using the Euler–Lagrange equation and a closure analysis, the authors establish a discrete biparametric family of closed, non-CMC rotational biconservative hypersurfaces in for every , none embedding. The results generalize known 3D classifications to arbitrary dimension and provide explicit closure criteria via the phase-integral .

Abstract

We characterise the profile curves of non-CMC biconservative rotational hypersurfaces of space forms as -elastic curves, for a suitable rational number which depends on the dimension of the ambient space. Analysing the closure conditions of these -elastic curves, we prove the existence of a discrete biparametric family of non-CMC closed (i.e., compact without boundary) biconservative hypersurfaces in . None of these hypersurfaces can be embedded in .
Paper Structure (7 sections, 11 theorems, 44 equations, 2 figures)

This paper contains 7 sections, 11 theorems, 44 equations, 2 figures.

Key Result

Theorem 2.1

Let $\varphi:M^{n-1}\rightarrow N^n$ be an isometric immersion with mean curvature function $H$. Then, the normal and tangential components of the Euler-Lagrange equation associated to the bienergy are, respectively, where $\eta$ is the unit normal vector field, $S_\eta$ is the shape operator and ${\rm Ric}$ denotes the Ricci curvature of $N^n$. Here, the symbol $\Delta$ represents the rough Lapl

Figures (2)

  • Figure 1: Closed $p$-elastic curves for the values $l=2$ and $r=3$ for different values of $p=(n-2)/(n+1)$. From left to right: $n=4$, $n=15$ and $n=30$.
  • Figure 2: Closed $p$-elastic curves for the values $l=3$ and $r=5$ for different values of $p=(n-2)/(n+1)$. From left to right: $n=4$, $n=15$ and $n=30$.

Theorems & Definitions (22)

  • Theorem 2.1
  • Proposition 2.2
  • Remark 3.1
  • Proposition 3.2
  • proof
  • Theorem 3.3
  • proof
  • Remark 3.4
  • Remark 3.5
  • Proposition 4.1
  • ...and 12 more