Primordial power spectrum from the dressed metric approach in loop cosmologies
Bao-Fei Li, Parampreet Singh, Anzhong Wang

TL;DR
This study compares the primordial power spectra predictions of three loop quantum cosmology models, analyzing how different regularizations and treatments affect the spectrum's amplitude across regimes.
Contribution
It provides a detailed comparison of standard and modified loop quantum cosmology models, highlighting the impact of regularizations and ambiguities on primordial spectra predictions.
Findings
Power spectrum is scale-invariant in the ultra-violet regime across all models.
Significant amplitude differences (up to 50%) occur in the infra-red and intermediate regimes.
Infra-red power spectrum magnitude in mLQC-I is of the order of the Planck scale.
Abstract
We investigate the consequences of different regularizations and ambiguities in loop cosmological models on the predictions in the scalar and tensor primordial spectrum of the cosmic microwave background using the dressed metric approach. Three models, standard loop quantum cosmology (LQC), and two modified loop quantum cosmologies (mLQC-I and mLQC-II) arising from different regularizations of the Lorentzian term in the classical Hamiltonian constraint are explored for chaotic inflation in spatially-flat Friedmann-Lema\^itre-Robertson-Walker (FLRW) universe. In each model, two different treatments of the conjugate momentum of the scale factor are considered. The first one corresponds to the conventional treatment in dressed metric approach, and the second one is inspired from the hybrid approach which uses the effective Hamiltonian constraint. For these two choices, we find the power…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
