activity
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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Showing 2017Show all

14 papers · 1 filter

astro-ph.CO2017★ 6 cited

Interaction in the dark sector: a Bayesian analysis with latest observations

T. Ferreira, C. Pigozzo, S. Carneiro +1

By combining cosmological probes at low, intermediate and high redshifts, we investigate the observational viability of a class of models with interaction in the dark sector. We pe…

gr-qc2017★ 37 cited

Screening mechanisms in hybrid metric-Palatini gravity

Marcelo Vargas dos Santos, Jailson S. Alcaniz, David F. Mota +1

We investigate the efficiency of screening mechanisms in the hybrid metric-Palatini gravity. The value of the field is computed around spherical bodies embedded in a background of…

astro-ph.CO2017★ 57 cited

The and tensions and the scale invariant spectrum

Micol Benetti, Leila L. Graef, Jailson S. Alcaniz

In a previous communication we showed that a joint analysis of Cosmic Microwave Background (CMB) data and the current measurement of the local expansion rate favours a model with a…

astro-ph.CO2017★ 38 cited

Isotropy of low redshift type Ia Supernovae: A Bayesian analysis

U. Andrade, C. A. P. Bengaly, J. S. Alcaniz +1

The standard cosmology strongly relies upon the Cosmological Principle, which consists on the hypotheses of large scale isotropy and homogeneity of the Universe. Testing these assu…

astro-ph.HE2017★ 140 cited

Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration

M. C. Díaz, L. M. Macri, D. Garcia Lambas +52

We present the results of prompt optical follow-up of the electromagnetic counterpart of the gravitational-wave event GW170817 by the Transient Optical Robotic Observatory of the S…

astro-ph.CO2017★ 25 cited

A Bayesian analysis of inflationary primordial spectrum models using Planck data

Simony Santos da Costa, Micol Benetti, Jailson Alcaniz

The current available CMB data show an anomalously low value of the CMB temperature fluctuations at large angular scales (l < 40). This lack of power is not explained by the minima…