DGP and DGPish cosmologies from actions
arXiv:2111.05061 · doi:10.1103/PhysRevD.105.083534
Abstract
In this work we explore and test new formulations of cosmological scenarios in theories. In these settings, the non-metricity scalar () is the main source of gravity and Friedmann equations are modified to account for the associated degrees of freedom. This work focuses first on the derivation, and then theoretical and observational analysis of two such (new) exact cosmological models; they both display a non-standard behaviour in which an additional parameter encoding non-metricity effects acts in the fashion of a screened cosmological constant. One of the new settings has the same background evolution as the well know DGP cosmological model, while the other resembles the former considerably, although its origin is purely phenomenological. We use the Markov Chain Montecarlo method combined with standard statistical techniques to perform observational astrophysical tests relying upon background data, specifically these are Type Ia Supernovae luminosities and direct Hubble data (from cosmic clocks), along with Cosmic Microwave Background shift and Baryon Acoustic Oscillations data. In addition, we compute some of the cosmographic parameters and other discriminators with the purpose of refining our knowledge about these models in the light of their theoretical and observational signatures, and this allows for a better comparison with the (concordance) CDM setup. We conclude that these scenarios do not show signatures indicating a departure from the CDM behaviour.
13 pages, 4 figures, 2 tables
References in corpus (10)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- The Confrontation between General Relativity and Experiment
- Beyond the Cosmological Standard Model
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Accelerated Expansion of the Universe in Non-minimally Coupled Gravity
- Cosmography in gravity
- Observational constraints on cosmological solutions of theories
- Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation
- When Did Cosmic Acceleration Start ?
- The Dark Sector Cosmology
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- Bianchi type-I cosmological dynamics in gravity: a covariant approach
- A note on the junction conditions in f(Q)-gravity
- Can an Extra Degree of Freedom in Scalar-Tensor Non-Metricity Gravity Account for the Evolution of the Universe?
- Geometric acceleration in theories
- Insights in cosmology: the relevance of the connection