Cargando…
Back Reaction And Local Cosmological Expansion Rate
We calculate the back reaction of cosmological perturbations on a general relativistic variable which measures the local expansion rate of the Universe. Specifically, we consider a cosmological model in which matter is described by a single field. We analyze back reaction both in a matter dominated...
Autores principales: | Geshnizjani, G, Brandenberger, R H |
---|---|
Lenguaje: | eng |
Publicado: |
2002
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.66.123507 http://cds.cern.ch/record/548726 |
Ejemplares similares
-
Back reaction and the local cosmological expansion rate
por: Geshnizjani, G, et al.
Publicado: (2002) -
1st Iranian International School on Cosmology : Large Scale Structure Formation
por: Mansouri, Reza, et al.
Publicado: (2000) -
Lectures on cosmology: accelerated expansion of the Universe
por: Wolschin, Georg
Publicado: (2010) -
Accelerating cosmological expansion from shear and bulk viscosity
por: Floerchinger, Stefan, et al.
Publicado: (2014) -
Cosmological Constant and Local Gravity
por: Bernabeu, Jose, et al.
Publicado: (2009)