PIRSA:23100108

Video URL

https://pirsa.org/23100108

Understanding Dwarf Galaxy Evolution to understand Dark Matter

Munshi, F. (2023). Understanding Dwarf Galaxy Evolution to understand Dark Matter. Perimeter Institute for Theoretical Physics. https://pirsa.org/23100108

Munshi, Ferah. Understanding Dwarf Galaxy Evolution to understand Dark Matter. Perimeter Institute for Theoretical Physics, Oct. 24, 2023, https://pirsa.org/23100108 

          @misc{ scivideos_PIRSA:23100108,
            doi = {10.48660/23100108},
            url = {https://pirsa.org/23100108},
            author = {Munshi, Ferah},
            keywords = {Cosmology},
            language = {en},
            title = {Understanding Dwarf Galaxy Evolution to understand Dark Matter},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2023},
            month = {oct},
            note = {PIRSA:23100108 see, \url{https://scivideos.org/index.php/pirsa/23100108}}
          }

Ferah Munshi George Mason University

Talk numberPIRSA:23100108
DOI10.48660/23100108
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

Low mass galaxies challenge our picture of galaxy formation and are an intriguing laboratory for the study of star formation, feedback and dark matter physics. I will present results from high resolution, cosmological simulations that contain many (isolated) dwarf galaxies [the MARVEL dwarfs] as well as satellite dwarf galaxies [the DC Justice League]. Together, they create the largest collection of high-resolution simulated dwarf galaxies to date and the first flagship suite to resolve ultra-faint dwarf galaxies in multiple environments. This sample spans a wide range of physical (stellar and halo mass), and evolutionary properties (merger history). I will present results and predictions constraining star formation, feedback and dark matter physics soon testable by telescopes like JWST, Rubin's LSST and the Roman Space Telescope. Finally, I will present new work on measuring galaxy shapes and the diversity of rotation curves in the dwarf galaxy mass regime which may be used to distinguish dark matter model.

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Zoom link: https://pitp.zoom.us/j/99038411436?pwd=OFd1SEdUUXJkd0NLeWtrTUxGR0FCUT09