Observational constraints on the linear fluctuation growth rate

• Verfasst von: Di Porto, Cinzia [VerfasserIn]
• Verfasst von: Amendola, Luca [VerfasserIn]
• Titel: Observational constraints on the linear fluctuation growth rate
• Verf.angabe: 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
• Fussnoten: Gesehen am 15.11.2017
• Titel Quelle: Enthalten in: Physical review / D
• Jahr Quelle: 2008
• Band/Heft Quelle: 77(2008,8) Artikel-Nummer 083508, 7 Seiten
• ISSN Quelle: 1550-2368
• ISSN Quelle: 1089-4918
• DOI: doi:10.1103/PhysRevD.77.083508
• Datenträger: Online-Ressource
• Sprache: eng
• K10plus-PPN: 1565360605

Abstract

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 previous expressions reproduces the growth function in models that allow for a growth faster than standard, as for instance in interacting or scalar-tensor models. We use data from galaxy and Lyman-α power spectra to constrain the linear growth rate. We find γ=0.6+0.4−0.3 for the growth rate index and η=0.0+0.3−0.2 for the additional growth parameter we introduce.