Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology

Abstract

In light of the statistical performance of cosmological observations, in this work we present an improvement on the Gaussian reconstruction of the Hubble parameter data $H(z)$ from Cosmic Chronometers, Supernovae Type Ia and Clustering Galaxies in a model-independent way in order to use them to study new constraints in the Horndeski theory of gravity. First, we have found that the prior used to calibrate the Pantheon supernovae data significantly affects the reconstructions, leading to a 13$\sigma$ tension on the $H_0$ value. Second, according to the ${\chi }^2$-statistics, the reconstruction carried out by the Pantheon data calibrated using the $H_0$ value measured by The Carnegie-Chicago Hubble Program is the reconstruction which fits best the observations of Cosmic Chronometers and Clustering of Galaxies datasets. Finally, we use our reconstructions of $H(z)$ to impose model-independent constraints in dark energy scenarios as Quintessence and K-essence from general cosmological viable Horndeski models, landscape in where we found that a Horndeski model of the K-essence type can reproduce the reconstructions of the late expansion of the universe within 2$\sigma$.

arXiv comment22 pages, 5 figures, 6 tables. Version accepted in JCAP

References in corpus (69)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• A 2.4% Determination of the Local Value of the Hubble Constant
• In the Realm of the Hubble tension $-$ a Review of Solutions
• Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• Covariant Galileon
• Constraining Cosmological Parameters Based on Relative Galaxy Ages
• Dark Energy after GW170817: dead ends and the road ahead
• Strong constraints on cosmological gravity from GW170817 and GRB 170817A
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Dark Energy after GW170817 and GRB170817A
• Imperfect Dark Energy from Kinetic Gravity Braiding
• Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
• Horndeski theory and beyond: a review
• Cosmology Intertwined II: The Hubble Constant Tension
• The Effective Field Theory of Dark Energy
• Dynamical dark energy in light of the latest observations
• Cosmology Intertwined III: $f{\sigma }_8$ and $S_8$
• Reconstruction of dark energy and expansion dynamics using Gaussian processes
• Can interacting dark energy solve the $H_0$ tension?
• H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
• Galileon Cosmology
• Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$
• Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Elucidating $\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• A Hubble Diagram for Quasars
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
• Dark energy in Horndeski theories after GW170817: A review
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• Generalized Galileon cosmology
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• The Cardassian expansion revisited: constraints from updated Hubble parameter measurements and Type Ia Supernovae data
• Using H(z) data as a probe of the concordance model
• Gravity in the Era of Equality: Towards solutions to the Hubble problem without fine-tuned initial conditions
• Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
• Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
• Measuring cosmological parameters with Gamma-Ray Bursts
• Reconstructing Gravity on Cosmological Scales
• Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• Ginzburg-Landau Theory of Dark Energy: A Framework to Study Both Temporal and Spatial Cosmological Tensions Simultaneously
• The $H_0$ tension: $\Delta G_N$ vs. $\Delta N_{\mathrm{eff}}$
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• hi_class: Background Evolution, Initial Conditions and Approximation Schemes
• Do current cosmological observations rule out all Covariant Galileons?
• Constraining Teleparallel Gravity through Gaussian Processes
• Cosmological data favor Galileon ghost condensate over $\Lambda$CDM
• Gaussian processes reconstruction of dark energy from observational data
• The road ahead of Horndeski: cosmology of surviving scalar-tensor theories
• Modified gravity for surveys
• Nonparametric reconstruction of the cosmic expansion with local regression smoothing and simulation extrapolation
• Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales
• Dynamical complexity of the Teleparallel gravity cosmology
• The role of the tachyonic instability in Horndeski gravity
• Does $\Lambda$CDM really be in tension with the Hubble diagram data?
• Nonparametric reconstruction of the Om diagnostic to test LCDM
• Varying the Horndeski Lagrangian within the Palatini approach
• Theoretical priors in scalar-tensor cosmologies: Thawing quintessence
• Most general cubic-order Horndeski Lagrangian allowing for scaling solutions and the application to dark energy
• Constraints on dark energy models from the Horndeski theory
• Black holes in self-tuning cubic Horndeski cosmology

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• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
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• DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends
• Unveiling the Universe with Emerging Cosmological Probes
• Performance of Non-Parametric Reconstruction Techniques in the Late-Time Universe
• On the degeneracy between $f{\sigma }_8$ tension and its Gaussian process forecasting
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