9–11 de septiembre de 2019
Facultad de Ciencias Físicas, UCM
Europe/Madrid zona horaria

Environmental dependence of the dynamical properties of light-cone simulation dark matter haloes

10 sept 2019, 18:00
15m
M2 (Facultad de Ciencias Físicas, UCM)

M2

Facultad de Ciencias Físicas, UCM

Contributed talk Tuesday afternoon

Ponente

Sra. Maria Chira (National Observatory of Athens)

Descripción

We study the dependence of a variety of halo properties (shape, spin, virialisation status) on different environments in a whole-sky ΛCDM light-cone halo catalogue extending to z ∼ 0.65,CDM light-cone halo catalogue extending to z ∼ 0.65, 0.65, using a simple and well-defined halo isolation criterion. Using this definition of the environment we study if and how the DM halo-properties and their interrelations depend on their environment. We also study the relative orientations of the spin- and shape- vectors of DM halos with their isolation, as well as the alignment of the shape- and the spin- vectors of neighbouring DM halos for a vast range of separations. Lastly, we focus on halo pairs, which are encountered in a variety of isolation states in our catalogue and, specifically, we study how the shape- and spin- alignments of halo-pairs is dependent on the isolation of the pair. The latter can give insight in the formation and evolution of halos formed under the dynamical interaction of their nearest neighbour in a region devoid of other massive halos, i.e. not affected by the ambient tidal field.

Materiales de la presentación