In this paper, we study flat Lorentz surfaces in anti-de Sitter 3-space H-1(3)(-1) in terms of the second conformal structure. Those flat Lorentz surfaces can be represented in terms of a Lorentz holomorphic and a Lorentz anti-holomorphic data similarly to WeierstraB representation formula. An analogue of hyperbolic GauB map is considered for timelike surfaces in H-1(3)(-1) and the relationship between the conformality (or the holomorphicity) of hyperbolic GauB map and the flatness of a Lorentz surface is discussed. It is shown that flat Lorentz surfaces in H-1(3)(-1) are associated with a hyperbolic Monge-Ampere ere equation. It is also known that Monge-Ampere equation may be regarded as a 2-dimensional reduction of the Einstein\u27s field...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper we introduce the notion of pseudo-spherical normal Darboux images of curves on a timel...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper, we study flat Lorentz surfaces in anti-de Sitter 3-space H-1(3)(-1) in terms of the s...
It is shown that timelike surfaces of constant mean curvature ± in anti-de Sitter 3-space H3 1(−1) c...
Let R-1(3) be the Lorentzian 3-space with inner product (,). Let Q(3) be the conformal compactificat...
AbstractWe study the neutral Kähler metric on the space of time-like lines in Lorentzian E13, which ...
The Lamarle Formula is known as a relationship between the Gaussian curvature and the distribution p...
Let Q(3) be the common conformal compactification space of the Lorentzian space forms R-1(3), S-1(3)...
Abstract. We construct stationary flat three-dimensional Lorentzian manifolds with singu-larities th...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper we introduce the notion of pseudo-spherical normal Darboux images of curves on a timel...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
It is shown that spacelike surfaces of constant mean curvature ±1 (abbreviated as CMC ±1) in de Sitt...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper we introduce the notion of pseudo-spherical normal Darboux images of curves on a timel...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper, we study flat Lorentz surfaces in anti-de Sitter 3-space H-1(3)(-1) in terms of the s...
It is shown that timelike surfaces of constant mean curvature ± in anti-de Sitter 3-space H3 1(−1) c...
Let R-1(3) be the Lorentzian 3-space with inner product (,). Let Q(3) be the conformal compactificat...
AbstractWe study the neutral Kähler metric on the space of time-like lines in Lorentzian E13, which ...
The Lamarle Formula is known as a relationship between the Gaussian curvature and the distribution p...
Let Q(3) be the common conformal compactification space of the Lorentzian space forms R-1(3), S-1(3)...
Abstract. We construct stationary flat three-dimensional Lorentzian manifolds with singu-larities th...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper we introduce the notion of pseudo-spherical normal Darboux images of curves on a timel...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
It is shown that spacelike surfaces of constant mean curvature ±1 (abbreviated as CMC ±1) in de Sitt...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...
In this paper we introduce the notion of pseudo-spherical normal Darboux images of curves on a timel...
Graviational instantons, solutions to the Euclidean Einstein equations, with toplogy R3×S1 arise nat...