Machine learning cosmic backreaction and its effects on observations
arXiv:2305.01224 · doi:10.1103/PhysRevLett.130.201003
Abstract
Symbolic expressions for cosmic backreaction and mean redshift drift in a range of 2-region models in terms of average quantities are presented. The demonstration that these expressions can be obtained constitutes the opening of a new avenue towards understanding the effects of cosmic backreaction in our universe: With a symbolic expression for the redshift drift at hand, the redshift drift can be used to constrain cosmological parameters including the large-scale expansion rate and backreaction. In addition, by introducing symbolic expressions for cosmic backreaction, this quantity can be constrained with observations such as redshift-distance measures.
arXiv comment6 pages, 3 captioned figures. Accepted for publication in PRL. v2: Updated reference list. No other changes
References in corpus (21)
- In the Realm of the Hubble tension a Review of Solutions
- Cosmology Intertwined II: The Hubble Constant Tension
- On average properties of inhomogeneous fluids in general relativity I: dust cosmologies
- Dark energy from backreaction
- Exact solution to the averaging problem in cosmology
- Accelerated expansion from structure formation
- A new framework for analyzing the effects of small scale inhomogeneities in cosmology
- Is there proof that backreaction of inhomogeneities is irrelevant in cosmology?
- Light propagation in statistically homogeneous and isotropic dust universes
- How well is our universe described by an FLRW model?
- Multiscale cosmology and structure-emerging Dark Energy: A plausibility analysis
- On the curvature of the present-day Universe
- Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature
- Another look at redshift drift and the backreaction conjecture
- Examples of backreaction of small scale inhomogeneities in cosmology
- Observations in statistically homogeneous, locally inhomogeneous cosmological toy-models without FLRW backgrounds
- A Simple, Heuristic Derivation of our "No Backreaction" Results
- Multipole decomposition of redshift drift -- model independent mapping of the expansion history of the Universe
- Redshift drift as a model independent probe of dark energy
- Cosmic backreaction and the mean redshift drift from symbolic regression
- Accelerating expansion of the universe may be caused by inhomogeneities
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- Analyzing the 21-cm signal brightness temperature in the Universe with inhomogeneities
- Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities
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