activity
20062018
most citedInteracting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters

207 citations · 411 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2018★ 3 cited

Quintessence and tachyon dark energy in interaction with dark matter: Observational constraints and model selection

Sandro M. R. Micheletti

We derive two field theory models of interacting dark energy, one in which dark energy is associated with the quintessence and another in which it is associated with the tachyon. I…

gr-qc2011★ 16 cited

Exact cosmological solutions of models with an interacting dark sector

A. B. Pavan, Elisa G. M. Ferreira, Sandro M. R. Micheletti +2

In this work we extend the first order formalism for cosmological models that present an interaction between a fermionic and a scalar field. Cosmological exact solutions describing…

gr-qc2010★ 9 cited

Holographic field theory models of dark energy in interaction with dark matter

Sandro M. R. Micheletti

We discuss two lagrangian interacting dark energy models in the context of the holographic principle. The potentials of the interacting fields are constructed. The models are compa…

gr-qc2009★ 81 cited

Observational constraints on holographic tachyonic dark energy in interaction with dark matter

Sandro M. R. Micheletti

We discuss an interacting tachyonic dark energy model in the context of the holographic principle. The potential of the holographic tachyon field in interaction with dark matter is…

gr-qc2009★ 95 cited

A Field Theory Model for Dark Matter and Dark Energy in Interaction

Sandro Micheletti, Elcio Abdalla, Bin Wang

We propose a field theory model for dark energy and dark matter in interaction. Comparing the classical solutions of the field equations with the observations of the CMB shift para…

astro-ph2006★ 207 cited

Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters

Bin Wang, Jiadong Zang, Chi-Yong Lin +2

Several observational constraints are imposed on the interacting holographic model of Dark Energy and Dark Matter. First we use the age parameter today, as given by the WMAP result…