Journal Club » History » Version 35
« Previous -
Version 35/269
(diff) -
Next » -
Current version
Robert Suhada, 02/06/2013 01:27 PM
Journal Club¶
Time: Weekly - Friday, 14:00 - 15:30
Place: Seminar room - I13 - upstairs
Next paper - 08.02.12 - The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics¶
Emiliano Munari, Andrea Biviano, Stefano Borgani, Giuseppe Murante, Dunja Fabjan
(Submitted on 8 Jan 2013)
[Abridged] We present an analysis of the relation between the masses of cluster- and group-sized halos, extracted from $\Lambda$CDM cosmological N-body and hydrodynamic simulations, and their velocity dispersions, at different redshifts from $z=2$ to $z=0$. The main aim of this analysis is to understand how the implementation of baryonic physics in simulations affects such relation, i.e. to what extent the use of the velocity dispersion as a proxy for cluster mass determination is hampered by the imperfect knowledge of the baryonic physics. In our analysis we use several sets of simulations with different physics implemented. Velocity dispersions are determined using three different tracers, DM particles, subhalos, and galaxies.
We confirm that DM particles trace a relation that is fully consistent with the theoretical expectations based on the virial theorem and with previous results presented in the literature. On the other hand, subhalos and galaxies trace steeper relations, and with larger values of the normalization. Such relations imply that galaxies and subhalos have a $\sim10$ per cent velocity bias relative to the DM particles, which can be either positive or negative, depending on halo mass, redshift and physics implemented in the simulation.
We explain these differences as due to dynamical processes, namely dynamical friction and tidal disruption, acting on substructures and galaxies, but not on DM particles. These processes appear to be more or less effective, depending on the halo masses and the importance of baryon cooling, and may create a non-trivial dependence of the velocity bias and the $\soneD$--$\Mtwo$ relation on the tracer, the halo mass and its redshift.
These results are relevant in view of the application of velocity dispersion as a proxy for cluster masses in ongoing and future large redshift surveys.
http://arXiv.org/abs/1301.1682
Paper pool¶
Click here to add papers you'd like to discuss.
Click here to add interesting papers that are too off-topic or controversial for the journal club.
Video talks and lectures¶
Click here to add links to talks or lectures you recommend.