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2014 | OriginalPaper | Buchkapitel

Fluids in Cosmology

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Abstract

We review the role of fluids in cosmology by first introducing them in General Relativity and then by applying them to a FRW model of the Universe. We describe how relativistic and non-relativistic components evolve in the background dynamics.We also introduce scalar fields to show that they are able to yield an inflationary dynamics at very early times (inflation) and late times (quintessence). Then, we proceed to study the thermodynamical properties of the fluids and, lastly, its perturbed kinematics. We make emphasis on the constrictions of parameters by recent cosmological probes.

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Metadaten
Titel
Fluids in Cosmology
verfasst von
Jorge L. Cervantes-Cota
Jaime Klapp
Copyright-Jahr
2014
DOI
https://doi.org/10.1007/978-3-319-00191-3_4