Baryon bias and structure formation in an accelerating universe
In most models of dark energy the structure formation stops after the accelerated expansion begins. In contrast, we show that the coupling of dark energy to dark matter may induce the growth of perturbations even in the accelerated regime. In particular, we show that this occurs in the models propos...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
28 August 2002
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| In: |
Physical review. D, Particles, fields, gravitation, and cosmology
Year: 2002, Jahrgang: 66, Heft: 4 |
| ISSN: | 1550-2368 |
| DOI: | 10.1103/PhysRevD.66.043528 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.66.043528 Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.66.043528 
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| Verfasserangaben: | Luca Amendola and Domenico Tocchini-Valentini, Osservatorio Astronomico di Roma, Viale Frascati 33, 00040 Monte Porzio Catone Roma, Italy |
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Baryon bias and structure formation in an accelerating universe
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