Hubble Parameter Corrected Interactions in Cosmology
We make steps in a new direction by considering fluids with EoS of more general form F(ρ,P)=0. It is thought that there should be interaction between cosmic fluids, but this assumption for this stage carries only phenomenological character opening a room for different kinds of manipulations. In this...
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| Hlavní autoři: | , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Wiley
2014-01-01
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| Edice: | Advances in High Energy Physics |
| On-line přístup: | http://dx.doi.org/10.1155/2014/129085 |
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