SUMMARY
The probability that the Universe is absolutely flat is constrained by the Planck data, which provides high precision estimates for the Hubble constant (H0 = 67.3 ± 1.0 km s−1 Mpc−1) and matter density (Ωm = 0.315 ± 0.013). When combined with Baryon Acoustic Oscillation (BAO) measurements, these estimates improve to H0 = 67.6 ± 0.6 km s−1 Mpc−1 and Ωm = 0.310 ± 0.008. The Universe appears to be spatially flat to a 1σ accuracy of 0.25%, indicating that while the mean curvature parameter is close to zero, the probability of it being exactly flat is effectively zero due to the continuous prior used in Bayesian statistics.
PREREQUISITES
- Understanding of the base Cold Dark Matter (CDM) model
- Familiarity with Planck satellite data and its implications
- Knowledge of Bayesian statistics and its application in cosmology
- Basic grasp of cosmological parameters such as Hubble constant and matter density
NEXT STEPS
- Research the implications of the Planck 2015 Results XIII on cosmological models
- Study Bayesian inference techniques in the context of cosmological data analysis
- Explore the relationship between Hubble constant variations and curvature parameters
- Investigate alternative models of the Universe's geometry and their statistical interpretations
USEFUL FOR
Astronomers, cosmologists, and researchers interested in the geometric properties of the Universe and the statistical methods used to analyze cosmological data.