Measurement on the cosmic curvature using the Gaussian process method
arXiv:2007.05714 · doi:10.1093/mnras/stab1085
Abstract
Inflation predicts that the Universe is spatially flat. The Planck 2018 measurements of the cosmic microwave background anisotropy favour a spatially closed universe at more than 2 confidence level. We use model independent methods to study the issue of cosmic curvature. The method reconstructs the Hubble parameter from cosmic chronometers data with the Gaussian process method. The distance modulus is then calculated with the reconstructed function and fitted by type Ia supernovae data. Combining the cosmic chronometers and type Ia supernovae data, we obtain which is consistent with a spatially flat universe at the 2 confidence level. By adding the redshift space distortions data to the type Ia supernovae data with a proposed novel model independent method, we obtain and no deviation from CDM model is found.
6 figures, 1 table, MNRAS in press
References in corpus (16)
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
- CfA3: 185 Type Ia Supernova Light Curves from the CfA
- A general test of the Copernican Principle
- Dynamical Dark Energy or Simply Cosmic Curvature?
- Constraining cosmic curvature by using age of galaxies and gravitational lenses
- Growth factor parametrization in curved space
- Testing the cosmic curvature at high redshifts: the combination of LSST strong lensing systems and quasars as new standard candles
- Model-independent determination of curvature parameter by using and data pair from BAO measurement
- Machine Learning the Cosmic Curvature in a Model-independent Way
- Model-independent Constraints on Cosmic Curvature and Opacity
- Model-independent Distance Calibration and Curvature Measurement using Quasars and Cosmic Chronometers
- Dark energy and cosmic curvature: Monte-Carlo Markov Chain approach
- Current cosmological constraints on the curvature, dark energy and modified gravity
- Model-independent determination of cosmic curvature based on Padé approximation
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- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- Is the Observable Universe Consistent with the Cosmological Principle?
- Non-parametric spatial curvature inference using late-universe cosmological probes
- Cosmic chronometers to calibrate the ladders and measure the curvature of the Universe. A model-independent study
- Cosmological constraints on slow-roll inflation: an update
- Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
- Cosmic expansion parametrization: Implication for curvature and tension
- Model-independent constraints on and from the link between geometry and growth
- Constraining the curvature density parameter in cosmology
- Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
- Null test for cosmic curvature using Gaussian process
- Non-parametric reconstruction of cosmological observables using Gaussian Processes Regression
- The impact of the Universe's expansion rate on constraints on modified growth of structure
- Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
- Revisiting the epoch of cosmic acceleration
- Checking the second law at cosmic scales
- Potentialities of Hubble parameter and expansion rate function data to alleviate Hubble tension
- Non-parametric reconstructions of cosmic curvature: current constraints and forecasts
- Revisiting model-independent constraints on spatial curvature and cosmic ladders calibration: updated and forecast analyses
- Tilted non-spatially-flat inflation
- Cosmic curvature on large-scale structures with homogeneous dark energy
- High precision measurement of cosmic curvature: from gravitational waves and cosmic chronometer
- Results from Hubble parameter data: oscillating dark energy?