2014
DOI: 10.1088/0264-9381/31/10/105012
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Piecewise silence in discrete cosmological models

Abstract: We consider a family of cosmological models in which all mass is confined to a regular lattice of identical black holes. By exploiting the reflection symmetry about planes that bisect these lattices into identical halves, we are able to consider the evolution of a number of geometrically distinguished surfaces that exist within each of them. We find that the evolution equations for the reflection symmetric surfaces can be written as a simple set of Friedmann-like equations, with source terms that behave like a… Show more

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Cited by 27 publications
(46 citation statements)
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“…The black hole lattice universe is often used as one of tools to evaluate effects of local non-linear inhomogeneities on the global expansion. Recently, black hole lattice universe models have been revisited by several authors [2][3][4][5][6][7][8][9][10][11][12]. Time symmetric initial data for N-black hole systems on a virtual 3-sphere have been analyzed in Refs.…”
Section: Introductionmentioning
confidence: 99%
“…The black hole lattice universe is often used as one of tools to evaluate effects of local non-linear inhomogeneities on the global expansion. Recently, black hole lattice universe models have been revisited by several authors [2][3][4][5][6][7][8][9][10][11][12]. Time symmetric initial data for N-black hole systems on a virtual 3-sphere have been analyzed in Refs.…”
Section: Introductionmentioning
confidence: 99%
“…The existence of a radiation-like term has also been found previously in other models. Firstly, in the case of regularly arranged black holes in a lattice under reflective symmetric boundary conditions 14 , and secondly in the case of the short wavelength approximation for fluctuations around a background metric 15 .…”
Section: Resultsmentioning
confidence: 99%
“…(2.6)). The latter then turns out to be P (g) 29) and is timelike. As stated above, replacing in region IV u → u + and v → v + allows the extension of the metric to the whole spacetime ds 2 I = − 4dudv + dx 2 + dy 2 ,…”
Section: Colliding Gravitational Plane Wavesmentioning
confidence: 96%