Non-oscillating vacuum states and the quantum homogeneity and isotropy hypothesis in Loop Quantum Cosmology
Beatriz Elizaga Navascu\'es, Guillermo A. Mena Marug\'an, and Santiago, Prado

TL;DR
This paper examines whether the quantum homogeneity and isotropy hypothesis in Loop Quantum Cosmology can select vacuum states that produce non-oscillating power spectra, finding that these criteria are compatible.
Contribution
It clarifies the relationship between the QHIH and non-oscillatory vacuum states, highlighting a feasible way to satisfy both in LQC.
Findings
The original set of states satisfying QHIH can include non-oscillatory vacua.
The procedure for selecting vacua has an ununivocal step affecting the outcome.
Compatibility between QHIH and non-oscillatory vacua is possible within the analyzed framework.
Abstract
We study the compatibility of the quantum homogeneitiy and isotropy hypothesis (QHIH), proposed by Ashtekar and Gupt to restrict the choice of vacuum state for the cosmological perturbations in Loop Quantum Cosmology (LQC), with the requirement that the selected vacuum should lead to a power spectrum that does not oscillate. We inspect in close detail the procedure that these authors followed to construct a set of states satisfying the QHIH, and how a preferred vacuum can be determined within this set. We find a step that is not univocally specified in this procedure, in relation with the replacement of the set of states that was originally allowed by the QHIH with an alternative set that is more manageable. In fact, the first of these sets does not contain the state that has been used in most of the implementations of the QHIH to the analysis of the power spectrum of the perturbations…
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.
