Impact of generalized holonomy corrections on the cosmological primordial power spectra

The propagation of perturbations is studied with generalized holonomy corrections in a fully consistent way, ensuring that the deformed algebra of constraints remains closed. The primordial cosmological power spectra are calculated. It is shown that, although the detailed form of the correction does unavoidably impact the observables, the main known results of loop quantum cosmology are robust in this respect.

Automated summary

The propagation of perturbations is investigated in the context of generalized holonomy corrections, ensuring closure of the deformed algebra of constraints. The primordial cosmological power spectra are calculated, and it is demonstrated that while the specific form of the correction does affect observables, the main results of loop quantum cosmology remain robust.