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The holonomy correction is one of the main terms arising when implementingloop quantum gravity ideas at an effective level in cosmology. The recentconstruction of an anomaly free algebra has shown that the formalism used, upto now, to derive the primordial spectrum of fluctuations was not correct. Thisarticle aims at computing the tensor spectrum in a fully consistent way withinthis deformed and closed algebra.

Primordial tensor power spectrum in holonomy corrected Omega-LQC