Fully Loop-Quantum-Cosmology-corrected propagation of gravitational
  waves during slow-roll inflation
  The cosmological primordial power spectrum is known to be one of the most
promising observable to probe quantum gravity effects. In this article, we
investigate how the tensor power spectrum is modified by Loop Quantum Gravity
corrections. The two most important quantum terms, holonomy and inverse volume,
are explicitly taken into account in a unified framework. The equation of
propagation of gravitational waves is derived and solved for one set of
parameters.
