Observational constraints on the linear fluctuation growth rate
Many experiments in the near future will test dark energy through its effects on the linear growth of matter perturbations. It is therefore important to find simple and at the same time general parametrizations of the linear growth rate. We show that a simple fitting formula that generalizes previou...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
14 April 2008
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Physical review. D, Particles, fields, gravitation, and cosmology
Year: 2008, Jahrgang: 77, Heft: 8, Pages: 083508 |
| ISSN: | 1550-2368 |
| DOI: | 10.1103/PhysRevD.77.083508 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.77.083508 Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.77.083508 
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| Verfasserangaben: | Cinzia Di Porto, Dipartimento di Fisica ‘‘E. Amaldi,’’ Università degli studi ‘‘Roma Tre,’’ Via della Vasca Navale 84, 00146 Roma, Italy, Luca Amendola, INAF/Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monte Porzio Catone (Roma), Italy |
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Observational constraints on the linear fluctuation growth rate
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