Challenges for scaling cosmologies
A cosmological model that aims at solving the coincidence problem should show that dark energy and dark matter follow the same scaling solution from some time onward. At the same time, the model should contain a sufficiently long matter-dominated epoch that takes place before acceleration in order t...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
24 July 2006
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| In: |
Physical review. D, Particles, fields, gravitation, and cosmology
Year: 2006, Jahrgang: 74, Heft: 2, Pages: 023525 |
| ISSN: | 1550-2368 |
| DOI: | 10.1103/PhysRevD.74.023525 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.74.023525 Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.74.023525 
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| Verfasserangaben: | Luca Amendola, Miguel Quartin, Shinji Tsujikawa, and Ioav Waga |
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