The dimensionless age of the Universe: a riddle for our time
arXiv:1607.00002 · doi:10.3847/0004-637X/828/1/35
Abstract
We present the interesting coincidence of cosmology and astrophysics that points toward a dimensionless age of the universe H_0*t_0 that is close to one. Despite cosmic deceleration for 9 Gyr and acceleration since then, we find H_0t*_0 = 0.96 +/- 0.01 for the LCDM model that fits SN Ia data from Pan-STARRS, CMB power spectra, and baryon acoustic oscillations. Similarly, astrophysical measures of stellar ages and the Hubble constant derived from redshifts and distances point to H_0*t ~ 1.0 +/- 0.1$. The wide range of possible values for H_0*t_0 realized during comic evolution means that we live at what appears to be a special time. This "synchronicity problem" is not precisely the same as the usual Coincidence problem because there are combinations of Omega_Matter and Omega_Lambda for which the usual coincidence problem holds but for which H_0*t_0 is not close to 1.
arXiv comment14 pages, 12 figures. Accepted for publication in the Astrophysical Journal (ApJ)
References in corpus (20)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- emcee: The MCMC Hammer
- The Cosmological Constant
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- Cosmological Results from High-z Supernovae
- A Precise Distance Indicator: Type Ia Supernova Multicolor Light Curve Shapes
- The extreme r-element rich, iron-poor halo giant CS31082-001: Implications for the r-process site(s) and radioactive cosmochronology
- Distances, ages, and epoch of formation of globular clusters
- Discovery of HE 1523-0901, a Strongly r-Process Enhanced Metal-Poor Star with Detected Uranium
- The R_h = ct Universe
- HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
- The Cosmic Horizon
- A Lower Limit on the Age of the Universe
- Confined Population III Enrichment and the Prospects for Prompt Second-Generation Star Formation
- Three Ancient Halo Subgiants: Precise Parallaxes, Compositions, Ages, and Implications for Globular Clusters
- Benchmark stars for Gaia: fundamental properties of the Population II star HD140283 from interferometric, spectroscopic and photometric data
- Formation of the First Low-Mass Stars from Cosmological Initial Conditions
- Through the Looking Glass: Why the "Cosmic Horizon" is not a horizon
- Another coincidence problem for CDM?
Cited by in corpus (12)
- Gravitational echoes from macroscopic quantum gravity effects
- Searching for dark matter - dark energy interactions: going beyond the conformal case
- Accelerated and decelerated expansion in a causal dissipative cosmology
- Supernova Magnitude Evolution and PAge Approximation
- Estimated Age of the Universe in Fractional Cosmology
- Cosmic expansion with matter creation and bulk viscosity
- Dynamical systems analysis of the cubic galileon beyond the exponential potential and the cosmological analogue of the vDVZ discontinuity
- A More Accurate Parameterization based on cosmic Age (MAPAge)
- What if the universe expands linearly? A local general relativity to solve the "zero active mass" problem
- Is cosmic dynamics self-regulating?
- Revisiting dynamics of interacting quintessence
- Bouncing and coasting universe with exact quantum-classical correspondence