Interacting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models
Mauricio Cataldo, Patricio Mella, Paul Minning, Joel Saavedra

TL;DR
This paper explores power-law Friedmann-Robertson-Walker cosmological models with two interacting perfect fluids, showing how interactions can lead to accelerated expansion and mimic single-fluid solutions, unlike non-interacting cases.
Contribution
It provides a detailed analysis of interacting fluid scenarios in power-law FRW models, revealing conditions for acceleration and equivalence to single-fluid models.
Findings
Interacting fluids can produce accelerated expansion in flat FRW models.
Power-law solutions with interacting fluids can mimic single-fluid cosmologies.
Non-interacting fluids do not generally admit power-law solutions with similar properties.
Abstract
We provide a detailed description for power--law scaling Friedmann-Robertson-Walker cosmological scenarios dominated by two interacting perfect fluid components during the expansion. As a consequence of the mutual interaction between the two fluids, neither component is conserved separately and the energy densities are proportional to . It is shown that in flat FRW cosmological models there can exist interacting superpositions of two perfect fluids (each of them having a positive energy density) which accelerate the expansion of the universe. In this family there also exist flat power law cosmological scenarios where one of the fluids may have a ``cosmological constant" or "vacuum energy" equation of state () interacting with the other component; this scenario exactly mimics the behavior of the standard flat Friedmann solution for a single fluid with a barotropic…
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