Comparing Analytic and Numerical Studies of Tensor Perturbations in Loop Quantum Cosmology
Guillermo A. Mena Marug\'an, Antonio Vicente-Becerril, Jes\'us, Y\'ebana Carrilero

TL;DR
This paper compares analytic and numerical methods for studying tensor perturbations in Loop Quantum Cosmology, focusing on different quantization approaches and vacuum choices to accurately compute the primordial power spectrum.
Contribution
It introduces a comprehensive comparison of hybrid and dressed metric approaches and validates analytic approximations against numerical results for tensor perturbations.
Findings
Analytic approximations closely match numerical results.
Hybrid and dressed metric approaches yield similar power spectra.
The NO-AHD vacuum effectively removes oscillations in the spectrum.
Abstract
We investigate the implications of different quantization approaches in Loop Quantum Cosmology for the primordial power spectrum of tensor modes. Specifically, we consider the hybrid and dressed metric approaches to derive the effective mass that governs the evolution of the tensor modes. Our study comprehensively examines the two resulting effective masses and how to estimate them in order to obtain approximated analytic solutions to the tensor perturbation equations. Since Loop Quantum Cosmology incorporates preinflationary effects in the dynamics of the perturbations, we do not have at our disposal a standard choice of privileged vacuum, like the Bunch--Davies state in quasi-de Sitter inflation. We then select the vacuum state by a recently proposed criterion which removes unwanted oscillations in the power spectrum and guarantees an asymptotic diagonalization of the Hamiltonian in…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Black Holes and Theoretical Physics
