English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Piecewise Silence in Discrete Cosmological Models

MPS-Authors

Gregoris,  Daniele
AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)

1402.3201.pdf
(Preprint), 527KB

CQG_31_10_105012.pdf
(Any fulltext), 351KB

Supplementary Material (public)
There is no public supplementary material available
Citation

Clifton, T., Gregoris, D., & Rosquist, K. (2014). Piecewise Silence in Discrete Cosmological Models. Classical and quantum gravity, 31: 105012. doi:10.1088/0264-9381/31/10/105012.


Cite as: https://hdl.handle.net/11858/00-001M-0000-001A-0E4F-A
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 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".