Measuring the expansion of the universe
arXiv:2005.02278
Abstract
We draw a figure from where it is possible to measure the number of e-folds of expansion of the universe with a ruler. We find model independent bounds for the number of e-folds during inflation, reheating and radiation. We also give a lower bound to the size of the universe at the beginning of observable inflation. Finally, we show that consistency with a relevant diagram requires the existence of a new form of energy to drive the present expansion of the universe.
arXiv comment13 pages, 4 figures, 1 table. A new section has been added. Improved presentation. Misprints in Table I have been corrected. Version sent for publication
References in corpus (14)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Inflation Dynamics and Reheating
- How long before the end of inflation were observable perturbations produced?
- Nonperturbative Dynamics Of Reheating After Inflation: A Review
- First CMB Constraints on the Inflationary Reheating Temperature
- Reheating constraints to inflationary models
- Reheating predictions in single field inflation
- Inflation after WMAP3: Confronting the Slow-Roll and Exact Power Spectra with CMB Data
- Observing the Inflationary Reheating
- Inflation and the Scale Dependent Spectral Index: Prospects and Strategies
- Bayesian Analysis of Inflation II: Model Selection and Constraints on Reheating
- A Horizon Ratio Bound for Inflationary Fluctuations
- Reheating temperature from the CMB
- On Inflationary Scale, Reheating Scale and Pre-BBN Cosmology with Scalar Fields