Ancient Mean Curvature Flows and their Spacetime Tracks

Publikation: Working paperPreprintForskning

Standard

Ancient Mean Curvature Flows and their Spacetime Tracks. / Chini, Francesco; Møller, Niels Martin.

2019. s. 1-14.

Publikation: Working paperPreprintForskning

Harvard

Chini, F & Møller, NM 2019 'Ancient Mean Curvature Flows and their Spacetime Tracks' s. 1-14. <https://arxiv.org/pdf/1901.05481.pdf>

APA

Chini, F., & Møller, N. M. (2019). Ancient Mean Curvature Flows and their Spacetime Tracks. (s. 1-14). arXiv.org https://arxiv.org/pdf/1901.05481.pdf

Vancouver

Chini F, Møller NM. Ancient Mean Curvature Flows and their Spacetime Tracks. 2019, s. 1-14.

Author

Chini, Francesco ; Møller, Niels Martin. / Ancient Mean Curvature Flows and their Spacetime Tracks. 2019. s. 1-14 (arXiv.org).

Bibtex

@techreport{718903039e284a90adac550edcc97ca2,
title = "Ancient Mean Curvature Flows and their Spacetime Tracks",
abstract = "We study properly immersed ancient solutions of the codimension one mean curvature flow in n-dimensional Euclidean space, and classify the convex hulls of the subsets of space reached by any such flow. In particular, it follows that any compact convex ancient mean curvature flow can only have a slab, a halfspace or all of space as the closure of its set of reach. The proof proceeds via a bi-halfspace theorem (also known as a wedge theorem) for ancient solutions derived from a parabolic Omori-Yau maximum principle for ancient mean curvature flows.",
author = "Francesco Chini and M{\o}ller, {Niels Martin}",
year = "2019",
language = "English",
series = "arXiv.org",
pages = "1--14",
type = "WorkingPaper",

}

RIS

TY - UNPB

T1 - Ancient Mean Curvature Flows and their Spacetime Tracks

AU - Chini, Francesco

AU - Møller, Niels Martin

PY - 2019

Y1 - 2019

N2 - We study properly immersed ancient solutions of the codimension one mean curvature flow in n-dimensional Euclidean space, and classify the convex hulls of the subsets of space reached by any such flow. In particular, it follows that any compact convex ancient mean curvature flow can only have a slab, a halfspace or all of space as the closure of its set of reach. The proof proceeds via a bi-halfspace theorem (also known as a wedge theorem) for ancient solutions derived from a parabolic Omori-Yau maximum principle for ancient mean curvature flows.

AB - We study properly immersed ancient solutions of the codimension one mean curvature flow in n-dimensional Euclidean space, and classify the convex hulls of the subsets of space reached by any such flow. In particular, it follows that any compact convex ancient mean curvature flow can only have a slab, a halfspace or all of space as the closure of its set of reach. The proof proceeds via a bi-halfspace theorem (also known as a wedge theorem) for ancient solutions derived from a parabolic Omori-Yau maximum principle for ancient mean curvature flows.

M3 - Preprint

T3 - arXiv.org

SP - 1

EP - 14

BT - Ancient Mean Curvature Flows and their Spacetime Tracks

ER -

ID: 311222657