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dc.contributor.authorClifton, Ten_US
dc.contributor.authorGregoris, Den_US
dc.contributor.authorRosquist, Ken_US
dc.date.accessioned2016-11-22T11:50:57Z
dc.date.submitted2016-11-07T16:34:52.026Z
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/17812
dc.description20 pages, 1 figure
dc.description20 pages, 1 figureen_US
dc.description.abstractWe 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 set of interacting effective fluids. We then show that gravitational waves are effectively trapped within small chambers for all time, and are not free to propagate throughout the space-time. Each chamber therefore evolves as if it were in isolation from the rest of the universe. We call this phenomenon "piecewise silence".en_US
dc.format.extent105012 - ?en_US
dc.relation.ispartofClass. Quantum Grav.en_US
dc.rightsThis is a pre-copyedited, author-produced PDF of an article accepted for publication in Classical and Quantum Gravity following peer review. The version of record is available http://iopscience.iop.org/article/10.1088/0264-9381/31/10/105012/meta
dc.subjectgr-qcen_US
dc.subjectgr-qcen_US
dc.subjectastro-ph.COen_US
dc.titlePiecewise Silence in Discrete Cosmological Modelsen_US
dc.typeArticle
dc.rights.holder© 2014 IOP Publishing Ltd
dc.identifier.doi10.1088/0264-9381/31/10/105012en_US
pubs.author-urlhttp://arxiv.org/abs/1402.3201v2en_US
pubs.notesNo embargoen_US
pubs.publisher-urlhttp://dx.doi.org/10.1088/0264-9381/31/10/105012en_US
pubs.volume31en_US


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