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Backreaction in cosmology
S Schander, T Thiemann - Frontiers in Astronomy and Space …, 2021 - frontiersin.org
In this review, we investigate the question of backreaction in different approaches to
cosmological perturbation theory, and with a special focus on quantum theoretical aspects …
cosmological perturbation theory, and with a special focus on quantum theoretical aspects …
Spherical inhomogeneous solutions of Einstein and scalar–tensor gravity: A map of the land
We review spherical and inhomogeneous analytic solutions of the field equations of Einstein
and of scalar–tensor gravity, including Brans–Dicke theory, non-minimally (possibly …
and of scalar–tensor gravity, including Brans–Dicke theory, non-minimally (possibly …
Dark energy
Dark Energy - IOPscience Skip to content IOP Science home Accessibility Help Search all
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IOPscience content Search Article Lookup Select journal (required) Volume number: Issue …
Does the growth of structure affect our dynamical models of the Universe? The averaging, backreaction, and fitting problems in cosmology
Abstract Structure occurs over a vast range of scales in the Universe. Our large-scale
cosmological models are coarse-grained representations of what exists, which have much …
cosmological models are coarse-grained representations of what exists, which have much …
The non-linear matter and velocity power spectra in f(R) gravity
We study the matter and velocity divergence power spectra in af (R) gravity theory and their
time evolution measured from several large-volume N-body simulations with varying box …
time evolution measured from several large-volume N-body simulations with varying box …
Testing the Void against Cosmological data: fitting CMB, BAO, SN and H0
In this paper, instead of invoking Dark Energy, we try and fit various cosmological
observations with a large Gpc scale under-dense region (Void) which is modeled by a …
observations with a large Gpc scale under-dense region (Void) which is modeled by a …
Clues on void evolution–II. Measuring density and velocity profiles on SDSS galaxy redshift space distortions
Using the redshift space distortions of void–galaxy cross-correlation function we analyse the
dynamics of voids embedded in different environments. We compute the void–galaxy cross …
dynamics of voids embedded in different environments. We compute the void–galaxy cross …
(Mis) interpreting supernovae observations in a lumpy universe
Light from 'point sources' such as supernovae is observed with a beam width of the order of
the sources' size–typically less than 1 au. Such a beam probes matter and curvature …
the sources' size–typically less than 1 au. Such a beam probes matter and curvature …
Interpretation of the Hubble diagram in a nonhomogeneous universe
P Fleury, H Dupuy, JP Uzan - Physical Review D—Particles, Fields, Gravitation …, 2013 - APS
In the standard cosmological framework, the Hubble diagram is interpreted by assuming that
the light emitted by standard candles propagates in a spatially homogeneous and isotropic …
the light emitted by standard candles propagates in a spatially homogeneous and isotropic …
Cosmic backreaction and the mean redshift drift from symbolic regression
SM Koksbang - Physical Review D, 2023 - APS
The possibility of obtaining symbolic expressions for cosmic backreaction is explored
through a case study of so-called 2-region models. By using the publicly available symbolic …
through a case study of so-called 2-region models. By using the publicly available symbolic …