2017
DOI: 10.1038/s41598-017-08872-4
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Navigability of Random Geometric Graphs in the Universe and Other Spacetimes

Abstract: Random geometric graphs in hyperbolic spaces explain many common structural and dynamical properties of real networks, yet they fail to predict the correct values of the exponents of power-law degree distributions observed in real networks. In that respect, random geometric graphs in asymptotically de Sitter spacetimes, such as the Lorentzian spacetime of our accelerating universe, are more attractive as their predictions are more consistent with observations in real networks. Yet another important property of… Show more

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Cited by 6 publications
(6 citation statements)
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“…However, we always call it the hyperbolic random geometric graph. In a broader sense, our work is an addition to the developing literature on random structures of hyperbolic spaces (see [12,6,5,34,31,40,17,21]).…”
Section: Introductionmentioning
confidence: 99%
“…However, we always call it the hyperbolic random geometric graph. In a broader sense, our work is an addition to the developing literature on random structures of hyperbolic spaces (see [12,6,5,34,31,40,17,21]).…”
Section: Introductionmentioning
confidence: 99%
“…Perhaps the simplest example of a random spatial network [1][2][3][4][5][6][7][8][9] is the 1d random geometric graph (1d RGG) [10][11][12][13][14][15][16]. 1d problems are widely studied in order to first understand a simpler case, such as the Ising and Heisenberg models of magnetism studied by Ising and Hans Bethe in 1924 and 1931 respectively, in the later case resulting in the famous Bethe ansatz, as well as more modern examples of e.g.…”
Section: Introductionmentioning
confidence: 99%
“…Given that the class of "nice" d-dimensional manifolds as considered above includes d-dimensional spheres (having constant positive curvature) and d-dimensional Euclidean spaces (having zero curvature), it is natural to ask about random geometric graphs on negatively curved spaces. Such an investigation was initiated recently in [28] on hyperbolic spaces and even more recently in [16] on more general spaces such as Lorentzian manifolds. However, since the d-dimensional Poincaré ball is one of the canonical and well-understood models of non-Euclidean and non-compact spaces, we shall restrict our attention to the same.…”
Section: Introductionmentioning
confidence: 99%