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Testing decaying dark matter with the cosmic background radiation and the first stars

    SO(Colloquium).

    Tracy Slatyer (MIT)

    Abstract: 

    84% of the matter in the universe is “dark”, presently invisible to us except through its gravitational interactions. However, even a tiny fraction of dark matter decaying or annihilating into visible particles could have striking effects on the primordial history of our universe. I will describe how these effects could manifest in distortions to cosmic radiation backgrounds, and present a new analysis indicating that they could also modify the time of formation of the first stars.

    When: November 16, 2023, 3:00pm to 4:30pm
    Location&Place: IFT Seminar Room/Red Room