A Quasi-Static Approach to Structure Formation in Black Hole Universes
Autor: | Jessie Durk, Timothy Clifton |
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Jazyk: | angličtina |
Rok vydání: | 2017 |
Předmět: |
Physics
Structure formation Cosmology and Nongalactic Astrophysics (astro-ph.CO) Degree (graph theory) 010308 nuclear & particles physics Lattice (group) Structure (category theory) FOS: Physical sciences Astronomy and Astrophysics Scale (descriptive set theory) General Relativity and Quantum Cosmology (gr-qc) 16. Peace & justice Lambda 01 natural sciences Cosmology General Relativity and Quantum Cosmology Black hole Theoretical physics 0103 physical sciences 010306 general physics Astrophysics - Cosmology and Nongalactic Astrophysics |
Popis: | Motivated by the existence of hierarchies of structure in the Universe, we present four new families of exact initial data for inhomogeneous cosmological models at their maximum of expansion. These data generalise existing black hole lattice models to situations that contain clusters of masses, and hence allow the consequences of cosmological structures to be considered in a well-defined and non-perturbative fashion. The degree of clustering is controlled by a parameter $\lambda$, in such a way that for $\lambda \sim 0$ or $1$ we have very tightly clustered masses, whilst for $\lambda \sim 0.5$ all masses are separated by cosmological distance scales. We study the consequences of structure formation on the total net mass in each of our clusters, as well as calculating the cosmological consequences of the interaction energies both within and between clusters. The locations of the shared horizons that appear around groups of black holes, when they are brought sufficiently close together, are also identified and studied. We find that clustering can have surprisingly large effects on the scale of the cosmology, with models that contain thousands of black holes sometimes being as little as 30% of the size of comparable Friedmann models with the same total proper mass. This deficit is comparable to what might be expected to occur from neglecting gravitational interaction energies in Friedmann cosmology, and suggests that these quantities may have a significant influence on the properties of the large-scale cosmology. Comment: 33 pages, 10 figures, v2: matches published version, typos corrected |
Databáze: | OpenAIRE |
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