activity
20102021
most citedMatter in inhomogeneous loop quantum cosmology: the Gowdy model

44 citations · 50 across the 4 of their papers we have counts for

collaborators

10 papers

gr-qc2021

Non-oscillatory power spectrum from States of Low Energy in kinetically dominated early universes

Mercedes Martín-Benito, Rita B. Neves, Javier Olmedo

Recently, States of Low Energy (SLEs) have been proposed as viable vacuum states of primordial perturbations within Loop Quantum Cosmology (LQC). In this work we investigate the ef…

gr-qc2021

States of Low Energy in bouncing inflationary scenarios in Loop Quantum Cosmology

Mercedes Martín-Benito, Rita B. Neves, Javier Olmedo

In generic Friedmann-Lemaître-Robertson-Walker spacetimes, States of Low Energy (SLEs) are defined to minimize the regularized energy density smeared along the time-like curve of a…

gr-qc2020

The Effect of a positive cosmological constant on the bounce of Loop Quantum Cosmology

Mercedes Martín-Benito, Rita B. Neves

We provide an analytical solution to the quantum dynamics of a flat Friedmann-Lemaître- Robertson-Walker model with a massless scalar field in the presence of a small and positive…

hep-th2019

Unitary quantization of a charged scalar field and Schwinger effect

Luis J. Garay, Alberto García Martín-Caro, Mercedes Martín-Benito

Quantum field theory in curved spacetimes suffers in general from an infinite ambiguity in the choice of Fock representation and associated vacuum. In cosmological backgrounds, the…

gr-qc20195 cited

Solvable Loop Quantum Cosmology: domain of the volume observable and semiclassical states

Mercedes Martín-Benito, Rita B. Neves

The dynamics of a flat Friedmann-Lemaître-Robertson-Walker model minimally coupled to a massless scalar field has been intensively studied in the context of Loop Quantum Cosmology.…

math-ph2018

On the Uniqueness of the Fock Quantization of the Dirac Field in the Closed FRW Cosmology

Jerónimo Cortez, Ilda Inácio Rodrigues, Mercedes Martín-Benito +1

The Fock quantization of free fields propagating in cosmological backgrounds is in general not unambiguously defined due to the non-stationarity of the spacetime. For the case of a…