activity
20182025
most citedAffine quantisation of the Brans-Dicke theory: Smooth bouncing and the equivalence between the Einstein and Jordan frames

27 citations · 97 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2025

Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology

Emmanuel Frion, Mateo Pascual, Francesca Vidotto

In the framework of Loop Quantum Cosmology, we study a cosmological bouncing model with two fields that reproduce the desired features of the primordial power spectra. The model co…

astro-ph.CO2025★ 4 cited

On the Hamilton-Jacobi approach to inflation beyond slow roll

Danilo Artigas, Emmanuel Frion, Tays Miranda +2

The Hamilton-Jacobi approach is a powerful tool to describe super-Hubble dynamics during cosmological inflation in a non-linear way. A key assumption of this framework is to neglec…

gr-qc2024★ 1 cited

Primordial magnetogenesis in a bouncing model with dark energy

Marcus V. Bomfim, Emmanuel Frion, Nelson Pinto-Neto +1

We investigate primordial magnetogenesis within a quantum bouncing model driven by a scalar field, focusing on various non-minimal couplings between the electromagnetic field and t…

astro-ph.CO2023★ 15 cited

Bayesian analysis of a Unified Dark Matter model with transition: can it alleviate the tension?

Emmanuel Frion, David Camarena, Leonardo Giani +4

We consider cosmological models in which Dark Matter (DM) and Dark Energy (DE) are described by a single component, dubbed Unified Dark Matter (UDM) models, in which the DE-like pa…

quant-ph2021★ 1 cited

Quantum formalism on the plane: POVM-Toeplitz quantization, Naimark theorem and linear polarisation of the light

Roberto Beneduci, Emmanuel Frion, Jean-Pierre Gazeau +1

We investigate two aspects of the elementary example of POVMs on the Euclidean plane, namely their status as quantum observables and their role as quantizers in the integral quanti…

gr-qc2021★ 10 cited

Black Hole Shadow Drift and Photon Ring Frequency Drift

Emmanuel Frion, Leonardo Giani, Tays Miranda

The apparent angular size of the shadow of a black hole in an expanding Universe is redshift-dependent. Since cosmological redshifts change with time - known as the redshift drift…