# On the index of minimal hypersurfaces of spheres

**Authors:** Oscar M. Perdomo

arXiv: 1902.10801 · 2019-03-01

## TL;DR

This paper investigates the stability index of minimal hypersurfaces in spheres, providing conditions under which the index exceeds a known value, thereby supporting a conjecture about the minimal possible index for non-Clifford hypersurfaces.

## Contribution

It proves that if the average of the squared second fundamental form is small and pointwise bounds hold, then the hypersurface's index exceeds the conjectured minimal value.

## Key findings

- The index is greater than n+3 under certain integral and pointwise bounds.
- Small average of |A|^2 implies index exceeds n+3.
- Supports the conjecture that only Clifford hypersurfaces have index n+3.

## Abstract

Let $M\subset S^{n+1}\subset\mathbb{R}^{n+2}$ be a compact minimal hypersurface of the $n$-dimensional Euclidean unit sphere. Let us denote by $|A|^2$ the square of the norm of the second fundamental form and $J(f)=-\Delta f-nf-|A|^2f$ the stability operator. It is known that the index (the number of negative eigenvalues of $J$) is 1 when $M$ is a totally geodesic sphere, and it is $n+3$ when $M$ is a Clifford minimal hypersurface. It has been conjectured that for any other minimal hypersurface, the index must be greater than $n+3$. One partial result for this conjecture states that if the index is $n+3$ and $M$ is not Clifford, then $\int_M |A|^2<n|M|$ where $|M|$ is the $n$ dimensional volume of $M$. Somehow this partial result states that if the index of $M$ is $n+3$ then the average of the function $|A|^2$ needs to be small. In this note we prove that this average cannot be very small. We will show that for any pair of positive numbers $\delta_1$ and $\delta_2$ with $\delta_1+\delta_2=1$, if $\int_M |A|^2\le \delta_2 n|M|$ and $|A|^2(x)\le2n\delta_1$ for all $x\in M$, then the index of $M$ is greater than $n+3$.

## Full text

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## References

5 references — full list in the complete paper: https://tomesphere.com/paper/1902.10801/full.md

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Source: https://tomesphere.com/paper/1902.10801