7 citations · 12 across the 7 of their papers we have counts for
7 papers
Kinematic state of an interacting cosmology modeled with Chebyshev polynomials
Freddy Cueva Solano
In a spatially flat universe and for an interacting cosmology, we have reconstructed the interaction term, , between a cold dark matter (DM) fluid and a dark energy (DE) fluid,…
Signals on the power spectra of a cosmology modeled with Chebyshev polynomials
Freddy Cueva Solano
We present an interacting model with a phenomenological interaction, , between a cold dark matter (DM) fluid and a dark energy (DE) fluid, which takes a time-varying equat…
Modeling interacting dark energy models with Chebyshev polynomials: Exploring their constraints and effects
Freddy Cueva Solano
In this work, we examine the main cosmological effects derived from a time-varying coupling () between a dark matter (DM) fluid and a dark energy (DE) fluid with time-vary…
Exploring the effects of a double reconstruction on the growth rate of cosmic structure, using current observational data
Freddy Cueva Solano
Based on General Relativity (GR) we consider two different cosmological scenarios in where reconstruct the energy exchange (Q) between cold dark matter (DM) fluid and dark energy (…
Exploring the effects of a double reconstruction on the geometrical parameters of coupled models, using observational data
Freddy Cueva Solano
In this work we study the effects of the non-gravitational exchange energy (Q) between dark matter (DM) fluid and dark energy (DE) fluid on the background evolution of the cosmolog…
Reconstruction of the interaction term between dark matter and dark energy using SNe Ia, BAO, CMB, H(z) and X-ray gas mass fraction
Freddy Cueva Solano, Ulises Nucamendi
Recently, in [1] we developed a parametric reconstruction method to a homogeneous, isotropic and spatially flat Friedmann-Robertson-Walker (FRW) cosmological model filled of a flui…
Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
Freddy Cueva Solano, Ulises Nucamendi
We apply a parametric reconstruction method to a homogeneous, isotropic and spatially flat Friedmann-Robertson-Walker (FRW) cosmological model filled of a fluid of dark energy (DE)…