Abstract

Abstract Motivated by the classical Euler elastic curves, David A. Singer posed in 1999 the problem of determining a plane curve whose curvature is given in terms of its position. We propound the same question in the Lorentz-Minkowski plane, focusing on spacelike and timelike curves. In this article, we study those curves in L 2 {{\mathbb{L}}}^{2} whose curvature depends on the Lorentzian pseudodistance from the origin, and those ones whose curvature depends on the Lorentzian pseudodistance through the horizontal or vertical geodesic to a fixed lightlike geodesic. Making use of the notions of geometric angular momentum (with respect to the origin) and geometric linear momentum (with respect to the fixed lightlike geodesic), respectively, we get two abstract integrability results to determine such curves through quadratures. In this way, we find out several new families of Lorentzian spiral, special elastic and grim-reaper curves whose intrinsic equations are expressed in terms of elementary functions. In addition, we provide uniqueness results for the generatrix curve of the Enneper surface of second kind and for Lorentzian versions of some well-known curves in the Euclidean setting, like the Bernoulli lemniscate, the cardioid, the sinusoidal spirals and some non-degenerate conics. We are able to get arc-length parametrizations of them and they are depicted graphically.

Highlights

  • Singer proposed in 1999 the following problem: Can a plane curve be determined if its curvature is given in terms of its position?

  • This question was motivated by the fact that for the classical Euler elastic curves, their curvature is proportional to one of the coordinate functions

  • The first condition is interpreted geometrically as those curves whose curvature depends on the Lorentzian pseudodistance from the origin, and the second one as those ones whose curvature depends on the Lorentzian pseudodistance through the horizontal or vertical geodesic to a fixed lightlike geodesic

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Summary

Introduction

We pay attention to identify, compute and plot such examples We find out the Lorentzian versions of some classical interesting curves in the Euclidean context corresponding to the sinusoidal spirals, characterized in Corollary 5.1 by their geometric angular momentum (ρ) = λ ρn+1 (and curvature κ(ρ) = λρn−1), λ > 0, n+1 n ≠ 0, n ≠ −1 They include the Lorentzian counterparts of the Bernoulli lemniscate, the cardioid and some non-degenerate conics (Remark 5.1) for particular values of n.

Spacelike and timelike curves in the Lorentz-Minkowski plane
Lorentzian Norwich spiral and its generalizations
Lorentzian sinusoidal spirals
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