Inflationary spectra and observations in loop quantum cosmology
Gianluca Calcagni
TL;DR
This paper reviews recent advances in calculating inflationary observables within loop quantum cosmology, highlighting how quantum corrections affect large-scale spectra and are constrained by observational data.
Contribution
It presents new insights into how inverse-volume quantum corrections influence inflationary spectra in loop quantum cosmology.
Findings
Inverse-volume quantum corrections cause growth in large-scale power spectra.
Observational data constrain the magnitude of quantum corrections.
The review summarizes progress in linking quantum cosmology with observable inflationary features.
Abstract
We review some recent progress in the extraction of inflationary observables in loop quantum cosmology. Inverse-volume quantum corrections induce a growth of power in the large-scale cosmological spectra and are constrained by observations.
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