On the observational determination of squeezing in relic gravitational waves and primordial density perturbations
Sukanta Bose, L.P. Grishchuk

TL;DR
This paper develops a theory linking relic gravitational waves and density perturbations to quantum squeezing effects in the early Universe, providing analytical predictions for observable features in the cosmic microwave background.
Contribution
It introduces a new analytical framework connecting squeezing of primordial quantum states to observable CMB features, improving understanding of early Universe physics.
Findings
Analytical formula for peaks and dips in the angular power spectrum
Good agreement between predicted and observed spectral features
Primordial squeezing better explains CMB structure than plasma acoustic peaks
Abstract
We develop a theory in which relic gravitational waves and primordial density perturbations are generated by strong variable gravitational field of the early Universe. The generating mechanism is the superadiabatic (parametric) amplification of the zero-point quantum oscillations. The generated fields have specific statistical properties of squeezed vacuum quantum states. Macroscopically, squeezing manifests itself in a non-stationary character of variances and correlation functions of the fields, the periodic structures of the metric power spectra, and, as a consequence, in oscillatory behavior of the higher order multipoles C_l of the cosmic microwave background anisotropy. We start with the gravitational wave background and then apply the theory to primordial density perturbations. We derive an analytical formula for the positions of peaks and dips in the angular power spectrum…
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