… Subhorizon inhomogeneities contribute only perturbatively to the Newtonian … inhomogeneities.
Assuming we start in an almost-FLRW universe, these small-scale inhomogeneities can …

… observed today in our universe at horizon scales [1–4]. … starts, it rapidly inflates away any
inhomogeneities, in order to … universe will be increasingly dominated by inhomogeneities rather …

… into discrete inhomogeneities of … inhomogeneity, rather than treat them as initial data, it is
necessary (but not sufficient) to find mechanisms which can remove or considerably inflate the …

… , because the universe that we observe is in many ways very inhomogeneous. The stars, …
The energy stored in the false vacuum became larger and larger as the universe inflated. Then …

… spectrum for energy density inhomogeneities in a closed universe, we study a … inflating
closed de Sitter space derived from Hawking’s prescription that the quantum state of the universe …

… This is why we have proposed a more conservative explanation, ascribing the departure of
the observed universe from an Einstein-de Sitter model to the influence of inhomogeneities. …

… in an inhomogeneous rather than a homogeneous universe. … , implying an inhomogeneous
scalar field P and minimally … fields together vanishes as the universe inflates. This is due to …

… Our universe appears smooth and uniform because all inhomogeneities were stretched …
the computer shrank down the original image, rather than expanding the inflating domains.) …

… inhomogeneous universe models and argue that, already in the absence of sources, an
effective scalar field arises through foliating and spatially averaging inhomogeneous … universe …

… inflationary universe. We show that the main fraction of volume of the Universe in a state …
If one assumes that we are typical observers living in the Universe at a given moment of time…