activity
20042021
most citedBeyond CDM: Problems, solutions, and the road ahead

530 citations · 1.1k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2021★ 12 cited

Structure formation in an anisotropic universe: Eulerian perturbation theory

Juan P. Beltrán Almeida, Josué Motoa-Manzano, Jorge Noreña +2

We present an effective Eulerian description, in the non-relativistic regime, of the growth of cosmological perturbations around a homogeneous but anisotropic Bianchi I spacetime b…

gr-qc2020★ 22 cited

Anisotropic solid dark energy

J. Motoa-Manzano, J. Bayron Orjuela-Quintana, Thiago S. Pereira +1

In this paper, we study a triad of inhomogeneous scalar fields, known as "solid", as a source of homogeneous but anisotropic dark energy. By using a dynamical system approach, we f…

astro-ph.CO2020★ 5 cited

Optimal Boltzmann hierarchies with non-vanishing spatial curvature

Cyril Pitrou, Thiago S. Pereira, Julien Lesgourgues

Within cosmological perturbation theory, the cosmic microwave background anisotropies are usually computed from a Boltzmann hierarchy coupled to the perturbed Einstein equations. I…

gr-qc2019★ 10 cited

Extended FLRW Models: dynamical cancellation of cosmological anisotropies

Mikjel Thorsrud, Ben D. Normann, Thiago S. Pereira

We investigate a corner of the Bianchi models that has not received much attention: "extended FLRW models" (eFLRW) defined as a cosmological model with underlying anisotropic Bianc…

gr-qc2019★ 8 cited

Beyond scalar, vector and tensor harmonics in maximally symmetric three-dimensional spaces

Cyril Pitrou, Thiago S. Pereira

We present a comprehensive construction of scalar, vector and tensor harmonics on maximally symmetric three-dimensional spaces. Our formalism relies on the introduction of spin-wei…

gr-qc2019★ 12 cited

Bianchi spacetimes as super-curvature modes around isotropic cosmologies

Thiago S. Pereira, Cyril Pitrou

A powerful result in theoretical cosmology states that a subset of anisotropic Bianchi models can be seen as the homogeneous limit of (standard) linear cosmological perturbations.…

astro-ph.CO2018★ 7 cited

CMB statistical isotropy confirmation at all scales using multipole vectors

Renan A. Oliveira, Thiago S. Pereira, Miguel Quartin

We present an efficient numerical code and conduct, for the first time, a null and model-independent CMB test of statistical isotropy using Multipole Vectors (MVs) at all scales. B…

astro-ph.CO2018★ 9 cited

Topology and the suppression of CMB large-angle correlations

Armando Bernui, Camila P. Novaes, Thiago S. Pereira +1

To date, no compelling evidence has been found that the universe has non-trivial spatial topology. Meanwhile, anomalies in the observed CMB temperature map, such as the lack of cor…

astro-ph.CO2018★ 32 cited

Direction and redshift drifts for general observers and their applications in cosmology

Oton H. Marcori, Cyril Pitrou, Jean-Philippe Uzan +1

High precision astrometry now enables to measure the time drift of astrophysical observables in real time, hence providing new ways to probe different cosmological models. This art…

gr-qc2016★ 10 cited

Two-point Correlation Functions in Inhomogeneous and Anisotropic Cosmologies

Oton H. Marcori, Thiago S. Pereira

Two-point correlation functions are ubiquitous tools of modern cosmology, appearing in disparate topics ranging from cosmological inflation to late-time astrophysics. When the back…

gr-qc2016★ 4 cited

Extending the LCDM model through shear-free anisotropies

Thiago S. Pereira, Davincy T. Pabon

If the spacetime metric has anisotropic spatial curvature, one can afford to expand the universe isotropically, provided that the energy-momentum tensor satisfy a certain con- stra…

astro-ph.CO2015★ 530 cited

Beyond CDM: Problems, solutions, and the road ahead

Philip Bull, Yashar Akrami, Julian Adamek +37

Despite its continued observational successes, there is a persistent (and growing) interest in extending cosmology beyond the standard model, CDM. This is motivated by a range o…

astro-ph.CO2015★ 22 cited

Isotropization of the universe during inflation

Thiago S. Pereira, Cyril Pitrou

A primordial inflationary phase allows one to erase any possible anisotropic expansion thanks to the cosmic no-hair theorem. If there is no global anisotropic stress, then the anis…

astro-ph.CO2015★ 3 cited

New Geometric Representations of the CMB 2pcf

Andre L. Froes, Thiago S. Pereira, Armando Bernui +1

When searching for deviations of statistical isotropy in CMB, a popular strategy is to write the two-point correlation function (2pcf) as the most general function of four spherica…

astro-ph.CO2015★ 14 cited

Cosmological Signatures of Anisotropic Spatial Curvature

Thiago S. Pereira, Guillermo A. Mena Marugán, Saulo Carneiro

If one is willing to give up the cherished hypothesis of spatial isotropy, many interesting cosmological models can be developed beyond the simple anisotropically expanding scenari…

astro-ph.CO2015★ 18 cited

Weak-lensing -modes as a probe of the isotropy of the universe

Thiago S. Pereira, Cyril Pitrou, Jean-Philippe Uzan

We compute the angular power spectrum of the -modes of the weak-lensing shear in a spatially anisotropic spacetime. We find that there must also exist off-diagonal correlations…

astro-ph.CO2015★ 32 cited

Weak-lensing by the large scale structure in a spatially anisotropic universe: theory and predictions

Cyril Pitrou, Thiago S. Pereira, Jean-Philippe Uzan

This article details the computation of the two-point correlators of the convergence, - and -modes of the cosmic shear induced by the weak-lensing by large scale structure as…

gr-qc2014★ 17 cited

Thermodynamics of quantum photon spheres

M. C. Baldiotti, Walace S. Elias, C. Molina +1

Photon spheres, surfaces where massless particles are confined in closed orbits, are expected to be common astrophysical structures surrounding ultracompact objects. In this paper…

astro-ph.CO2014★ 21 cited

North-South non-Gaussian asymmetry in PLANCK CMB maps

A. Bernui, A. F. Oliveira, T. S. Pereira

We report the results of a statistical analysis performed with the four foreground-cleaned Planck maps by means of a suitably defined {\it local-variance} estimator. Our analysis s…

astro-ph.CO2013

Inflationary Super-Hubble Waves and the Size of the Universe

Thiago S. Pereira, Luis Gustavo T. Silva

The effect of the scalar spectral index on inflationary super-Hubble waves is to amplify/damp large wavelengths according to whether the spectrum is red () or blue ($n_{s}…

astro-ph.CO2012★ 11 cited

Real Space Approach to CMB deboosting

Amanda Yoho, Craig J. Copi, Glenn D. Starkman +1

The effect of our Galaxy's motion through the Cosmic Microwave Background rest frame, which aberrates and Doppler shifts incoming photons measured by current CMB experiments, has b…

astro-ph.CO2012★ 16 cited

Inflationary Perturbations in Anisotropic, Shear-Free Universes

Thiago S. Pereira, Saulo Carneiro, Guillermo A. Mena Marugan

In this work, the linear and gauge-invariant theory of cosmological perturbations in a class of anisotropic and shear-free spacetimes is developed. After constructing an explicit s…

astro-ph.CO2012★ 23 cited

Weak lensing B-modes on all scales as a probe of local isotropy

Cyril Pitrou, Jean-Philippe Uzan, Thiago S. Pereira

This article derives a multipolar hierarchy for the propagation of the weak-lensing shear and convergence in a general spacetime. The origin of B-modes, in particular on large angu…

astro-ph.CO2010★ 10 cited

Effects of a Cut, Lorentz-Boosted sky on the Angular Power Spectrum

Thiago S. Pereira, Amanda Yoho, Maik Stuke +1

The largest fluctuation in the observed CMB temperature field is the dipole, its origin being usually attributed to the Doppler Effect - the Earth's velocity with respect to the CM…