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PreprintarXiv licencearXiv

Instability of mean curvature flow in expander coordinates

Abstract

We study rotationally symmetric graphical solutions to mean curvature flow that are initially close to a homothetic reference expander, in particular near infinity. Based on a computer algebra aided proof, we show that under appropriate conditions, at large times, the solutions are closer to a different expander than to the reference expander.

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BibTeX
@misc{lambert2026instability,
  title = {{Instability of mean curvature flow in expander coordinates}},
  author = {Ben S. Lambert and Oliver C. Schnürer},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.32819},
  eprint = {2610.32819},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.32819},
}
RIS
TY  - UNPB
TI  - Instability of mean curvature flow in expander coordinates
AU  - Ben S. Lambert
AU  - Oliver C. Schnürer
PY  - 2026
DA  - 2026/10/23
PB  - arXiv
DO  - 10.48550/arxiv.2610.32819
UR  - https://arxiv.org/abs/2610.32819
AB  - We study rotationally symmetric graphical solutions to mean curvature flow that are initially close to a homothetic reference expander, in particular near infinity. Based on a computer algebra aided proof, we show that under appropriate conditions, at large times, the solutions are closer to a different expander than to the reference expander.
ER  -