A new quantum-corrected mass function in loop quantum cosmology, with a free parameter xi, produces a wave-packet structure in the primordial power spectrum and matches the CMB angular spectrum best at xi = 0.2.
Hybrid quantization of an inflationary universe
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abstract
We quantize to completion an inflationary universe with small inhomogeneities in the framework of loop quantum cosmology. The homogeneous setting consists of a massive scalar field propagating in a closed, homogeneous scenario. We provide a complete quantum description of the system employing loop quantization techniques. After introducing small inhomogeneities as scalar perturbations, we identify the true physical degrees of freedom by means of a partial gauge fixing, removing all the local degrees of freedom except the matter perturbations. We finally combine a Fock description for the inhomogeneities with the polymeric quantization of the homogeneous background, providing the quantum Hamiltonian constraint of the composed system. Its solutions are then completely characterized, owing to the suitable choice of quantum constraint, and the physical Hilbert space is constructed. Finally, we consider the analog description for an alternate gauge and, moreover, in terms of gauge-invariant quantities. In the deparametrized model, all these descriptions are unitarily equivalent at the quantum level.
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The primordial angular power spectrum from the alternative mass function in loop quantum cosmology
A new quantum-corrected mass function in loop quantum cosmology, with a free parameter xi, produces a wave-packet structure in the primordial power spectrum and matches the CMB angular spectrum best at xi = 0.2.