25–27 Aug 2021
Online
Europe/Zurich timezone

Contribution List

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  1. Laura Sagunski (Goethe University Frankfurt), Sean Tulin (York University)
    25/08/2021, 16:00
  2. Darren Singh (York University), Hannah Vormann (Goethe University), Megan Gran (York University), Tobias Raum (Goethe University)
    25/08/2021, 16:15
    • Chair: Niklas Becker
    • Co-Chair: Saeed Rastgoo

    Mentor: Sean Tulin
    Junior mentor: Reuben Blaff

    Dark matter halos are a fundamental unit of structure in the Universe: from the very first stars born in small mini-halos, all the way up to the supermassive halos that hold together clusters of thousands of galaxies. This research will study how dark matter's particle dynamics – its...

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  3. Rebecca Leane (Massachusetts Institute of Technology)
    25/08/2021, 17:30
    • Chair: Laura Sagunski
    • Co-Chair: Nassim Bozorgnia

    Stars and planets can be ideal playgrounds to discover dark matter. In this talk, I will review a range of dark matter searches using celestial objects, including neutron stars, exoplanets, solar-system planets, and our Sun. I will discuss different search strategies, their opportunities and limitations, and the interplay of regimes...

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  4. 25/08/2021, 18:15
  5. Keiwan Jamaly (Goethe University), Lukas Hölker (Goethe University), Natey Kübler (Goethe University), Tarnem Afify (York University)
    26/08/2021, 16:00
    • Chair: Y. Fabian Bautista
    • Co-Chair: Nassim Bozorgnia

    Mentors: Laura Sagunski, Saeed Rastgoo
    Junior mentors: Niklas Becker, Julia Lienert

    Supermassive black holes at the centers of galaxies are surrounded by gigantic dark matter halos. Near these black holes, the dark matter density is extremely high and forms a so-called dark matter density spike. Due to its extremely high...

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  6. Diego Montalvo (York University), Ida Schmidt (Goethe University), Nour Khalil (York University)
    26/08/2021, 17:10
    • Chair: Alejandro Cruz-Osorio
    • Co-Chair: Jürgen Schaffner-Bielich

    Mentors: Laura Sagunski, Saeed Rastgoo
    Junior mentors: Niklas Becker, Julia Lienert

    Supermassive black holes at the centers of galaxies are surrounded by gigantic dark matter halos. Near these black holes, the dark matter density is extremely high and forms a so-called dark matter density spike. Due to its extremely...

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  7. Jürgen Schaffner-Bielich (Frankfurt University), Laura Sagunski (Goethe University Frankfurt), Nassim Bozorgnia, Saeed Rastgoo (York University), Sean Tulin (York University)
    26/08/2021, 18:15
  8. Andrew Robertson
    27/08/2021, 15:00
    • Chair: Nassim Bozorgnia
    • Co-Chair: Sean Tulin

    As the objects with the largest dark matter densities and velocity dispersions, galaxy clusters are an ideal laboratory in which to search for evidence of dark matter self-interactions. I will discuss how self-interacting dark matter (SIDM) is implemented within cosmological simulations, and then how comparing these simulations with...

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  9. Elham Rahimi (York University), Jasmin Hartmann (Goethe University), Lukas Arda (Goethe University)
    27/08/2021, 16:05
    • Chair: Reuben Blaff
    • Co-Chair: Sean Tulin

    Mentor: Nassim Bozorgnia
    Junior Mentor: Yilber Fabian Bautista

    In this project, we will use cosmological simulations of self-interacting dark matter (including baryons) to study the dark matter distribution in Milky Way–like galaxies. The complicated interplay between astrophysical processes and dark matter self-interactions can result in...

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  10. Alex Brisebois (University of Toronto), Marie Cassing (Goethe University), Muhammad Azeem (York University)
    27/08/2021, 17:05
    • Chair: Julia Lienert
    • Co-chair: Laura Sagunski

    Mentor: Jürgen Schaffner-Bielich
    Junior mentor: Alejandro Cruz-Osorio

    In this project, we explore the properties of astronomical objects which can be formed by dark matter and the properties of neutron stars in the presence of a dark matter component. First, we will get ourselves acquainted with the properties of interacting bosons...

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  11. 27/08/2021, 17:50