The inextricable bond between dark-matter halos and galaxies

Data: 
18/11/2020 - 14:00 - 15:00
Local: 
Remoto, com transmissão pela internet
The inextricable bond between dark-matter halos and galaxies
 
Antonio D. Montero-Dorta
 
IFUSP
 
A few hundred thousand years after the Big Bang, dark matter started to collapse slowly by the effect of its own gravity. As this process proceeded to form the virialized structures that we call dark-matter  halos, the increasing gravitational pull exerted by these objects  began to attract baryons into their potential wells. These baryons will later cool and condense, forming the seeds of the galaxies that we observe today. This primordial link between the baryonic and the dark-matter components dictates that the formation and evolution of galaxies cannot be fully understood unless their intricate relations with their hosting halos are taken into account. In this talk, I will summarize my recent contributions to the field of the halo-galaxy connection, which I address from the perspective of theory, modeling, and observations. I will focus on the effect called secondary halo bias, which refers to the dependence of the clustering of dark-matter halos on their multiple internal properties. I will discuss the physical origins of these secondary dependencies and their potential manifestation on the galaxy population.