Constraining Planck scale physics with CMB and Reionization Optical Depth
arXiv:1710.00759
Abstract
We present proof of principle for a two way interplay between physics at very early Universe and late time observations. We find a relation between primordial mechanisms responsible for large scale power suppression in the primordial power spectrum and the value of reionization optical depth . Such mechanisms can affect the estimation of . We show that using future measurements of , one can obtain constraints on the pre-inflationary dynamics, providing a new window on the physics of the very early Universe. Furthermore, the new, re-estimated can potentially resolve moderate discrepancy between high and low- measurements of , hence providing empirical support for the power suppression anomaly and its primordial origin.
5 pages, 3 figures
References in corpus (18)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Loop Quantum Cosmology: A Status Report
- Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization
- Quantum Nature of the Big Bang
- Planck 2013 results. XXIII. Isotropy and statistics of the CMB
- CMB-S4 Science Book, First Edition
- The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations
- A Quantum Gravity Extension of the Inflationary Scenario
- Does the small CMB quadrupole moment suggest new physics?
- Punctuated inflation and the low CMB multipoles
- Eliminating the optical depth nuisance from the CMB with 21 cm cosmology
- Getting Around Cosmic Variance
- Phenomenological investigation of a quantum gravity extension of inflation with the Starobinsky potential
- Low-l CMB Power Loss in String Inflation
- Pre-slow roll initial conditions: large scale power suppression and infrared aspects during inflation
- New model of axion monodromy inflation and its cosmological implications