Combined constraints on deviations of dark energy from an ideal fluid from Euclid and Planck
Cosmological fluids are commonly assumed to be distributed in a spatially homogeneous way, while their internal properties are described by a perfect fluid. As such, they influence the Hubble-expansion through their respective densities and equation of state parameters. The subject of this paper is...
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| Main Authors: | , , |
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| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
16 June 2015
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1506.04609
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| Author Notes: | Elisabetta Majerotto, Domenico Sapone and Björn Malte Schäfer |
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