Real- and redshift-space halo clustering in f(R) cosmologies.
Arnalte-Mur, P.; Hellwing, W.A.; Norberg, P.;
- Publisher: Oxford University Press
- Journal: volume 467,pagesstx196-1,585issn: 0035-8711, eissn: 1365-2966
- Subject: STFC | data analysis [methods] | large-scale structure of Universe [cosmology] | ST/K00042X/1 | ST/H008519/1 | dark energy [cosmology] | Astrophysics - Cosmology and Nongalactic Astrophysics | theory [cosmology] | RCUK | gravitation | ST/K003267/1 | ST/L00075X/1arxiv: Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Galaxy Astrophysics
We present two-point correlation function statistics of the mass and the halos in the chameleon $f(R)$ modified gravity scenario using a series of large volume N-body simulations. Three distinct variations of $f(R)$ are considered (F4, F5 and F6) and compared to a fiduc... View more