Exploring the liminality: properties of haloes and subhaloes in borderline f(R) gravity release_3znun32n6rgi5fhp265o6zefsu

by Difu Shi, Jiaxin Han (ICC, Durham), Liang Gao, Wojciech A. Hellwing (ICC, Durham)

Released as a article .

2015  

Abstract

We investigate the properties of dark matter haloes and subhaloes in an f(R) gravity model with |f_R0|=10^-6, using a very high-resolution N-body simulation. The model is a borderline between being cosmologically interesting and yet still consistent with current data. We find that the halo mass function in this model has a maximum 20 ΛCDM predictions between z=1 and z=0. Because of the chameleon mechanism which screens the deviation from standard gravity in dense environments, haloes more massive than 10^13h^-1M_ in this f(R) model have very similar properties to haloes of similar mass in ΛCDM, while less massive haloes, such as that of the Milky Way, can have steeper inner density profiles and higher velocity dispersions due to their weaker screening. The halo concentration is remarkably enhanced for low-mass haloes in this model due to a deepening of the total gravitational potential. Contrary to the naive expectation, the halo formation time z_f is later for low-mass haloes in this model, a consequence of these haloes growing faster than their counterparts in ΛCDM at late times and the definition of z_f. Subhaloes, especially those less massive than 10^11h^-1M_, are substantially more abundant in this f(R) model for host haloes less massive than 10^13h^-1M_. We discuss the implications of these results for the Milky Way satellite abundance problem. Although the overall halo and subhalo properties in this borderline f(R) model are close to their ΛCDM predictions, our results suggest that studies of the Local Group and astrophysical systems, aided by high-resolution simulations, can be valuable for further tests of it.
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Stage   accepted
Date   2015-07-09
Version   v2
Language   en ?
arXiv  1503.01109v2
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