Theory Seminar (High Energy/Cosmology)

<< Summer 2022 Fall 2022 Spring 2023 >>
Subscribe your calendar or receive email announcements of events

Events During the Week of November 27th through December 4th, 2022

Monday, November 28th, 2022

No events scheduled

Tuesday, November 29th, 2022

Dark Matter Substructure: simulations, semi-analytic models and observations
Time: 4:00 pm
Place: Chamberlin 5280
Speaker: Xiaolong Du, Carnegie Observatories & UCLA
Abstract: Roughly 85% of the matter in the Universe is in the form of invisible matter, i.e. dark matter. Under gravitational interactions, dark matter clusters and forms hierarchical structure. Over the last decades, simulations with higher and higher resolutions have greatly improved our understanding of the formation of dark matter halos and the properties of their substructure (subhalo). Simulations of the standard cold dark matter (CDM) show that CDM halos have cuspy density profiles and contain a large number of small subhalos, which are not fully consistent with the current observations of dwarf galaxies. Thus different dark matter models, such as warm dark matter, self-interacting dark matter, fuzzy dark matter, have been proposed, which predict very different phenomena on small scales (~kpc). Running numerical simulations under different dark matter assumptions requires a large amount of computing resource. On the hand, even the state-of-art simulations suffer from numerical artifacts, limiting their predicting power on small scales. In this talk, I will talk about some of our latest progresses in modeling the evolution of subhalos using the semi-analytic code Galacticus and how we can model and control the numerical artifacts. Using our semi-analytic models, we can get accurate predictions for the abundance of subhalos and the evolution of their density profiles due to tidal effects. Our semi-analytic models are ~10^4 times faster than direct simulations, making it possible to generate a large number of realizations of dark matter halo systems with correct substructure, which are useful for getting robust constraint on different dark matter models from observations such as strong gravitational lensing.
Host: George Wojcik
Add this event to your calendar

Wednesday, November 30th, 2022

No events scheduled

Thursday, December 1st, 2022

No events scheduled

Friday, December 2nd, 2022

No events scheduled