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19992023
most citedEnergy conditions in f(R)-gravity

296 citations · 6.5k across the 170 of their papers we have counts for

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78 papers · 1 filter

astro-ph.CO2023★ 16 cited

The miniJPAS survey: clusters and galaxy groups detection with AMICO

M. Maturi, A. Finoguenov, P. A. A. Lopes +31

Samples of galaxy clusters allow us to better understand the physics at play in galaxy formation and to constrain cosmological models once their mass, position (for clustering stud…

astro-ph.CO2023★ 8 cited

Forecasting constraints on the baryon mass fraction in the IGM from fast radio bursts and type Ia supernovae

Thais Lemos, Rodrigo S. Gonçalves, Joel C. Carvalho +1

Fast Radio Bursts (FRBs) are millisecond transient radio events with a high energy. By identifying the origin of the \textbf{burst}, it is possible to measure the redshift of the h…

astro-ph.CO2023★ 4 cited

Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation

F. B. M. dos Santos, R. Silva, J. S. Alcaniz

We investigate the impact of a non-minimal coupling of the scalar field with gravity in inflationary models, where a small coupling is allowed. As a concrete example, we consider t…

astro-ph.CO2023★ 27 cited

Low-redshift estimates of the absolute scale of baryon acoustic oscillations

Thais Lemos, Ruchika, Joel C. Carvalho +1

Measurements of the characteristic length scale of the baryon acoustic oscillations (BAO) provide a robust determination of the distance-redshift relation. Currently, the bes…

astro-ph.CO2023★ 6 cited

Higgs Inflation: constraining the top quark mass and breaking the - correlation

Jamerson G. Rodrigues, Micol Benetti, Rayff de Souza +1

Extending previous results [JHEP 11 (2021) 091], we explore aspects of the reheating mechanism for non-minimal Higgs inflation in the strong coupling regime. We constrain the radia…

astro-ph.CO2022★ 1 cited

The Hubble Constant Troubled by Dark Matter in Non-Standard Cosmologies

Jailson S. Alcaniz, Jacinto P. Neto, Farinaldo S. Queiroz +2

The Standard Cosmological Model has experienced tremendous success at reproducing observational data by assuming a universe dominated by a cosmological constant and dark matter in…

astro-ph.CO2022★ 21 cited

Measuring the Hubble Constant with cosmic chronometers: a machine learning approach

Carlos Bengaly, Maria Aldinez Dantas, Luciano Casarini +1

Local measurements of the Hubble constant () based on Cepheids e Type Ia supernova differ by from the estimated value of from Planck CMB observations under…

astro-ph.CO2022

Warm -exponential inflation and the Swampland Conjectures

F. B. M. dos Santos, R. Silva, S. Santos da Costa +2

We investigate theoretical and observational aspects of a warm inflation scenario driven by the -exponential potential, which generalizes the well-known power law inflation. In…

astro-ph.CO2022★ 11 cited

One-parameter dynamical dark-energy from the generalized Chaplygin gas

Rodrigo von Marttens, Dinorah Barbosa, Jailson Alcaniz

The fact that Einstein's equations connect the space-time geometry to the total matter content of the cosmic substratum, but not to individual contributions of the matter species,…

astro-ph.CO2022★ 13 cited

Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data

Thais Lemos, Rodrigo S. Gonçalves, Joel C. Carvalho +1

Fast Radio Bursts (FRBs) are millisecond-duration radio transients with an observed dispersion measure () greater than the expected Milky Way contribution, which suggests that…

astro-ph.CO2022

The angular scale of homogeneity with SDSS-IV DR16 Luminous Red Galaxies

Uendert Andrade, Rodrigo S. Gonçalves, Gabriela C. Carvalho +3

We report measurements of the angular scale of cosmic homogeneity () using the recently released luminous red galaxy sample of the sixteenth data release of the Sloan Digita…

astro-ph.CO2021★ 16 cited

A Test of the Standard Cosmological Model with Geometry and Growth

Uendert Andrade, Dhayaa Anbajagane, Rodrigo von Marttens +2

We perform a general test of the and cosmological models by comparing constraints on the geometry of the expansion history to those on the growth of stru…

astro-ph.CO2021★ 51 cited

Testing the consistency between cosmological data: the impact of spatial curvature and the dark energy EoS

Javier E. Gonzalez, Micol Benetti, Rodrigo von Marttens +1

The results of joint analyses of available cosmological data have motivated an important debate about a possible detection of a non-zero spatial curvature. If confirmed, such a res…

astro-ph.CO2021★ 30 cited

J-PAS: Forecasts for dark matter - dark energy elastic couplings

David Figueruelo, Miguel Aparicio Resco, Florencia A. Teppa Pannia +21

We consider a cosmological model where dark matter and dark energy feature a coupling that only affects their momentum transfer in the corresponding Euler equations. We perform a f…

astro-ph.CO2021★ 35 cited

Dark sector interactions and the curvature of the Universe in light of Planck's 2018 data

Micol Benetti, Humberto Borges, Cassio Pigozzo +2

We investigate the observational viability of a class of interacting dark energy (iDE) models in the light of the latest Cosmic Microwave Background (CMB), type Ia supernovae (SNe)…

astro-ph.CO2021★ 23 cited

J-PAS: forecasts on interacting vacuum energy models

V. Salzano, C. Pigozzo, M. Benetti +21

The next generation of galaxy surveys will allow us to test some fundamental aspects of the standard cosmological model, including the assumption of a minimal coupling between the…

astro-ph.CO2020★ 31 cited

A model-independent reconstruction of dark sector interactions

Rodrigo von Marttens, Javier E. Gonzalez, Jailson Alcaniz +2

Relaxing the conventional assumption of a minimal coupling between the dark matter (DM) and dark energy (DE) fields introduces significant changes in the predicted evolution of the…

astro-ph.CO2020★ 27 cited

Measuring the cosmic homogeneity scale with SDSS-IV DR16 Quasars

Rodrigo S. Gonçalves, Gabriela C. Carvalho, Uendert Andrade +3

We report measurements of the scale of cosmic homogeneity () using the recently released quasar sample of the sixteenth data release of the Sloan Digital Sky Survey (SDSS-IV…

astro-ph.CO2020★ 9 cited

Thermodynamic Constraints on the Dark Sector

W. J. C. da Silva, J. E. Gonzalez, R. Silva +1

In this paper, we present a unified scheme based on the fluid description of the dark sector of the universe. The scheme captures models with interaction between dark energy and da…

astro-ph.CO2020★ 119 cited

The miniJPAS survey: a preview of the Universe in 56 colours

S. Bonoli, A. Marín-Franch, J. Varela +166

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique…

astro-ph.CO2020★ 12 cited

Is there evidence for a hotter Universe?

Carlos A. P. Bengaly, Javier E. Gonzalez, Jailson S. Alcaniz

The measurement of present-day temperature of the Cosmic Microwave Background (CMB), K (1), made by the Far-InfraRed Absolute Spectrophotometer (FIRA…

astro-ph.CO2020★ 22 cited

Observational constraints on -attractor inflationary models with a Higgs-like potential

J. G. Rodrigues, S. Santos da Costa, J. S. Alcaniz

We investigate the observational viability of a class of -attractors inflationary models in light of the most recent Cosmic Microwave Background (CMB) and Large-Scale Structure…

astro-ph.CO2020★ 14 cited

Brane inflation and the robustness of the Starobinsky inflationary model

S. Santos da Costa, M. Benetti, R. M. P. Neves +3

The first inflationary model conceived was the one proposed by Starobinsky which includes an additional term quadratic in the Ricci-scalar R in the Einstein-Hilbert action. The mod…

astro-ph.CO2020★ 17 cited

Probing the Seesaw Mechanism with Cosmological Data

J. G. Rodrigues, Micol Benetti, Marcela Campista +1

We investigate cosmological consequences of an inflationary model which incorporates a generic seesaw extension (types I and II) of the Standard Model of Particle Physics. A non-mi…