Evidence of dark energy in different cosmological observations

Abstract

The idea of a negative-pressure dark energy component in the Universe which causes an accelerated expansion in the late Universe has deep implications in models of field theory and general relativity. In this article, we survey the evidence for dark energy from cosmological observations which started from the compilation of distance-luminosity plots of Type Ia supernovae. This turned out to be consistent with the dark energy inferred from the CMB observations and large scale surveys and gave rise to the concordance $\Lambda$CDM model of cosmology. In this article, we discuss the observational evidence for dark energy from Type Ia supernovae, CMB, galaxy surveys, observations of the Sunyaev-Zeldovich effect from clusters, and lensing by clusters. We also discuss the observational discrepancy in the values of $H_0$ and ${\sigma }_8$ between CMB and large scale structures and discuss if varying dark energy models are able to resolve these tensions between different observations.

arXiv commentA mini review to apear in EPJST (18 pages, 4 figures)

References in corpus (83)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Exploring the Expansion History of the Universe
• Accelerating Universes with Scaling Dark Matter
• The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
• Stable clustering, the halo model and nonlinear cosmological power spectra
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
• Toward a halo mass function for precision cosmology: the limits of universality
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
• Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Weak Gravitational Lensing of the CMB
• Early Dark Energy Can Resolve The Hubble Tension
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
• Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
• BVRI Light Curves for 22 Type Ia Supernovae
• First-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters
• CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
• CfA3: 185 Type Ia Supernova Light Curves from the CfA
• Dynamical dark energy in light of the latest observations
• The Sloan Digital Sky Survey-II Supernova Survey: Technical Summary
• SNLS3: Constraints on Dark Energy Combining the Supernova Legacy Survey Three Year Data with Other Probes
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey - Imaging Data and Catalogue Products
• Large-scale instability in interacting dark energy and dark matter fluids
• Early dark energy, the Hubble-parameter tension, and the string axiverse
• The DESI Experiment, a whitepaper for Snowmass 2013
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
• UBVRI Light Curves of 44 Type Ia Supernovae
• The Carnegie Supernova Project: First Photometry Data Release of Low-Redshift Type Ia Supernovae
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Cosmological Constraints from Measurements of Type Ia Supernovae discovered during the first 1.5 years of the Pan-STARRS1 Survey
• The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae
• Early Dark Energy Does Not Restore Cosmological Concordance
• The ESSENCE Supernova Survey: Survey Optimization, Observations, and Supernova Photometry
• H0 Revisited
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
• Indications of a late-time interaction in the dark sector
• Cosmological implications of ultra-light axion-like fields
• The Bispectrum as a Signature of Gravitational Instability in Redshift-Space
• The Carnegie Supernova Project: Second Photometry Data Release of Low-Redshift Type Ia Supernovae
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate
• Constraining Early Dark Energy with Large-Scale Structure
• Resolving the Hubble Tension with New Early Dark Energy
• CfA4: Light Curves for 94 Type Ia Supernovae
• The Data Release of the Sloan Digital Sky Survey-II Supernova Survey
• Reconciling CMB and structure growth measurements with dark energy interactions
• Evidence for anisotropy of cosmic acceleration
• KiDS-450: Testing extensions to the standard cosmological model
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe
• Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• Examining the evidence for dynamical dark energy
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Coupled dark matter-dark energy in light of near Universe observations
• Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
• Density perturbations for running vacuum: a successful approach to structure formation and to the ${\sigma }_8$-tension
• Constraints on dark energy with the LOSS SN Ia sample
• New Early Dark Energy is compatible with current LSS data
• Formulae for Growth Factors In Expanding Universes Containing Matter and a Cosmological Constant
• Theoretical uncertainty in baryon oscillations
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
• Relaxing the ${\sigma }_8$-tension through running vacuum in the Universe
• Testing Dark energy models in the light of ${\sigma }_8$ tension
• Neutrino mass and dark energy constraints from redshift-space distortions
• Quantifying the Redshift Space Distortion of the Bispectrum II: Induced Non-Gaussianity at Second Order Perturbation
• Cosmological constrains on minimally and non-minimally coupled scalar field models
• Dark Matter - Dark Energy coupling biasing parameter estimates from CMB data
• A model independent parametrization of the late time cosmic acceleration: constraints on the parameters from recent observations

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