Structure formation in the Deser-Woodard nonlocal gravity model: a reappraisal
In this work, we extend previous analyses of the structure formation in the f ( ##IMG## [http://ej.iop.org/icons/Entities/square.gif] square −1 R ) model of nonlocal gravity proposed by Deser and Woodard (DW), which reproduces the background expansion of ΛCDM with no need of a cosmological constant...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
27 April 2017
|
| In: |
Journal of cosmology and astroparticle physics
Year: 2017, Heft: 4, Pages: 1-11 |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2017/04/046 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1088/1475-7516/2017/04/046 Verlag, Volltext: http://stacks.iop.org/1475-7516/2017/i=04/a=046 
|
| Verfasserangaben: | Henrik Nersisyan, Adrian Fernandez Cid and Luca Amendola |
| Zusammenfassung: | In this work, we extend previous analyses of the structure formation in the f ( ##IMG## [http://ej.iop.org/icons/Entities/square.gif] square −1 R ) model of nonlocal gravity proposed by Deser and Woodard (DW), which reproduces the background expansion of ΛCDM with no need of a cosmological constant nor of any dimensional constant beside Newton's one. A previous analysis based on redshift-space distortions (RSD) data concluded that the model was ruled out. In this work we revisit the issue and find that, when recast in a localized model, the DW model is not ruled out and actually gives a better fit to RSD data than ΛCDM. In fact, the DW model presents a suppressed growth of matter perturbations with respect to ΛCDM and a slightly lower value of σ 8 , as favored by observations. We also produce analytical approximations of the two modified gravity functions, i.e. the anisotropic stress η and the relative change of Newton's constant Y , and of f σ 8 ( z ) as a function of redshift. Finally, we also show how much the fit depends on initial conditions when these are generalized with respect to a standard matter-dominated era. |
|---|---|
| Beschreibung: | Gesehen am 19.09.2017 |
| Beschreibung: | Online Resource |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2017/04/046 |