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...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
Wiley
2014-01-01
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| Σειρά: | Advances in High Energy Physics |
| Διαθέσιμο Online: | http://dx.doi.org/10.1155/2014/129085 |
| Ετικέτες: |
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