activity
20052025
most citedNon-adiabatic dark fluid cosmology

75 citations · 154 across the 9 of their papers we have counts for

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Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO2025

Cosmological Remapping for Efficient Generation of 21 cm Intensity Mapping Mocks

Rahima Mokeddem, Bruno B. Bizarria, Jiajun Zhang +10

We present a novel application of cosmological rescaling, or "remapping," to generate 21 cm intensity mapping mocks for different cosmologies. The remapping method allows for compu…

astro-ph.CO2025

Probing cosmic isotropy: Hubble constant and matter density large-angle variations with the Pantheon+SH0ES data

Rahima Mokeddem, Maria Lopes, Felipe Avila +2

In this study we investigate potential large-angle anisotropies in the angular distribution of the cosmological parameters (the Hubble constant) and (the matter density…

astro-ph.CO2022★ 13 cited

Excess of lensing amplitude in the Planck CMB power spectrum

Rahima Mokeddem, Wiliam S. Hipólito-Ricaldi, Armando Bernui

Precise measurements of the Planck cosmic microwave background (CMB) angular power spectrum (APS) at small angles have stimulated accurate statistical analyses of the lensing ampli…

astro-ph.CO2017

On general features of warm dark matter with reduced relativistic gas

W. S. Hipolito-Ricaldi, R. F. vom Marttens, J. C. Fabris +2

Reduced Relativistic Gas (RRG) is a useful approach to describe the warm dark matter (WDM) or the warmness of baryonic matter in the approximation when the interaction between the…

astro-ph.CO2017★ 2 cited

Does a generalized Chaplygin gas correctly describe the cosmological dark sector?

R. F. vom Marttens, L. Casarini, W. Zimdahl +2

Yes, but only for a parameter value that makes it almost coincide with the standard model. We reconsider the cosmological dynamics of a generalized Chaplygin gas (gCg) which is spl…

astro-ph.CO2016★ 24 cited

CMB and matter power spectra with non-linear dark-sector interactions

R. F. vom Marttens, L. Casarini, W. S. Hipólito-Ricaldi +1

An interaction between dark matter and dark energy, proportional to the product of their energy densities, results in a scaling behavior of the ratio of these densities with respec…