2019
DOI: 10.1016/j.aim.2019.06.015
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Polynomial quadratic differentials on the complex plane and light-like polygons in the Einstein Universe

Abstract: We construct geometrically a homeomorphism between the moduli space of polynomial quadratic differentials on the complex plane and light-like polygons in the 2-dimensional Einstein Universe. As an application, we find a class of minimal Lagrangian maps between ideal polygons in the hyperbolic plane.

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Cited by 11 publications
(21 citation statements)
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“…By definition, this means that the equivariant maximal embeddings associated to (h,q) and (h,q) have the same holonomy representation and the same boundary at infinity. On the other hand, the same argument as in [, Lemma 4.2] shows that given a locally achronal curve normalΓ in normalAdS3 the maximal surface bounding normalΓ is unique. This gives a contradiction because the pair (h,q) is uniquely determined by the embedding data of the maximal surface.…”
Section: Parameterising Regular Anti‐de Sitter Structuresmentioning
confidence: 69%
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“…By definition, this means that the equivariant maximal embeddings associated to (h,q) and (h,q) have the same holonomy representation and the same boundary at infinity. On the other hand, the same argument as in [, Lemma 4.2] shows that given a locally achronal curve normalΓ in normalAdS3 the maximal surface bounding normalΓ is unique. This gives a contradiction because the pair (h,q) is uniquely determined by the embedding data of the maximal surface.…”
Section: Parameterising Regular Anti‐de Sitter Structuresmentioning
confidence: 69%
“…If the induced metric is complete, the space‐like condition implies that, identifying AdŜ3 with D×S1 via F, the surface is the graph of a 2‐Lipschitz map [, Proposition 3.1] and its boundary at infinity normalΓ is a topological circle in normalAdS3 [, Corollary 3.3]. We also have control on the causal geometry of the curve at infinity.…”
Section: Background Materialsmentioning
confidence: 99%
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