5–9 Dec 2022
Australia/Sydney timezone

Session

Plenary

5 Dec 2022, 09:15
G03 (Ainsworth Building)

G03

Ainsworth Building

Conveners

Plenary

  • Matthew Dolan (University of Melbourne)

Plenary

  • Ciaran O'Hare (Sydney)

Plenary

  • Nicole Bell (The University of Melbourne)

Plenary

  • Archil Kobakhidze

Plenary

  • Alejandro Ibarra

Plenary

  • Danny Marfatia

Plenary

  • Osamu Seto

Plenary

  • Masahiro Kawasaki

Plenary

  • Chris Gordon (University of Canterbury)

Plenary

  • Sven Heinemeyer (CSIC (Madrid, ES))

Description

Livestream link: https://tinyurl.com/DSU2022plenary

Presentation materials

There are no materials yet.

  1. 05/12/2022, 09:15
  2. Joerg Jaeckel (Institut fuer theoretische Physik, Heidelberg University)
    05/12/2022, 09:30
    Plenary
  3. Dr Florian Kühnel (LMU Munich)
    05/12/2022, 10:00
    Plenary
  4. Adam Ritz
    05/12/2022, 11:00
    Plenary
  5. Theresa Fruth (University of Sydney)
    05/12/2022, 11:30
    Plenary
  6. Elisabetta Barberio
    05/12/2022, 12:00
    Plenary
  7. Natsumi Nagata
    06/12/2022, 09:00
    Plenary
  8. Aaron Vincent (Queen's University)
    06/12/2022, 09:30
    Plenary
  9. Geraint Lewis
    06/12/2022, 10:00
    Plenary

    Our view of the stellar halos of large galaxies is being revolutionised as deep surveys reveal a wealth of stellar streams and shells.As the remnants of progenitors that have been tidally disrupted in the galactic potential, this stellar debris offers the promise of determining the dark matter properties of the halo. Here, I will review the current state of the field, and provide a panoramic...

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  10. Alexander Vikman (Czech Academy of Sciences (CZ))
    06/12/2022, 11:00
    Plenary

    I will discuss a recently proposed class of models where Dark Matter (DM) is produced via an inverse phase transition. The inverse phase transition can be caused by coupling to some cosmological field. For instance, this field can be a primordial magnetic field, as in e-Print: 2010.03383 or thermal fluctuations of other fields, as in e-Print: 2104.13722. In the latter work DM is modelled as a...

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  11. Shinji Mukohyama
    06/12/2022, 11:30
    Plenary
  12. Bin Hu (Beijing Normal University)
    06/12/2022, 12:00
    Plenary
  13. Prof. Raymond Volkas (The University of Melbourne)
    07/12/2022, 09:00
    Plenary
  14. Julia Harz
    07/12/2022, 09:30
    Plenary
  15. Sunny Seo
    07/12/2022, 10:00
    Plenary

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  16. Valentina De Romeri
    07/12/2022, 11:00
    Plenary

    I will present the physics potential of the coherent elastic neutrino-nucleus scattering (CEvNS) process. I will first briefly review the status of current observations. Then I will comment about their implications for both precision tests of the Standard Model and for new physics in the neutrino sector. Finally I will discuss the relevance of these measurements for direct dark matter detection probes.

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  17. Meng-Ru Wu (Institute of Physics, Academia Sinica)
    07/12/2022, 11:30
    Plenary
  18. Jenni Adams (University of Canterbury)
    07/12/2022, 12:00
    Plenary

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  19. Tony Gherghetta (University of Minnesota (US))
    08/12/2022, 09:00
    Plenary
  20. Yann MAMBRINI
    08/12/2022, 09:30
    Plenary

    I will present in this talk recent works concerning the production of
    particles in the earliest stage of the Universe, between the preheating phase and the reheating time. I will insist on the subtleties of backreactions from scattering of the inflaton and apply it to the mechanism to the dark matter production in minimal extensions of the Standard Model, especially gravitational production.

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  21. Prof. Pyungwon Ko (KIAS)
    08/12/2022, 10:00
    Plenary
  22. Jinn-Ouk Gong
    08/12/2022, 11:00
    Plenary

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  23. Sachiko Kuroyanagi (IFT UAM-CSIC)
    08/12/2022, 11:30
    Plenary
  24. Prof. Yu-Feng Zhou
    08/12/2022, 12:00
    Plenary
  25. Roland Crocker
    09/12/2022, 09:00
    Plenary

    The Fermi Bubbles are giant, γ-ray emitting lobes emanating from the nucleus of the Milky Way discovered in ∼1-100 GeV data collected by the Large Area Telescope on board the Fermi Gamma-Ray Space Telescope. Previous work has revealed substructure within the Fermi Bubbles that has been interpreted as a signature of collimated outflows from the Galaxy’s super-massive black hole. Here we show...

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  26. Dr Gavin Rowell
    09/12/2022, 09:30
    Plenary

    Gamma-rays are a high effective tracer of extreme particle acceleration in the cosmos and can also be used to probe fundamental, beyond-standard-model and exotic physics in the present and in the early Universe. In this talk, I will summarise some recent results in gamma-ray astronomy from the current generation of ground-based facilities (e.g. HESS, MAGIC, VERITAS, HAWC, LHAASO) focusing on...

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  27. Tracy Slatyer
    09/12/2022, 10:00
    Plenary
  28. Prof. Cora Dvorkin
    09/12/2022, 11:00
    Plenary
  29. Csaba Balazs
    09/12/2022, 11:30
    Plenary

    I give an update on results for dark matter obtained using GAMBIT, the Global And Modular BSM Inference Tool. After briefly describing the main features of the GAMBIT code, I highlight why GAMBIT is a promising framework to isolate sign of physics beyond the standard models (BSM) of particle physics and cosmology. Then I show the latest GAMBIT results for various models containing a dark...

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  30. Keith A. Olive (University of Minnesota (US))
    09/12/2022, 12:00
    Plenary
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