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Sydney Spring School 2022

30 November 2022 to 2 December 2022
University of Sydney
Australia/Sydney timezone

Contribution List

24 out of 24 displayed
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  1. 6. Opening/Introductions
    30/11/2022, 09:45
  2. 1. Dark matter 1
    Yann MAMBRINI
    30/11/2022, 10:00
  3. 2. Dark matter 2
    Yann MAMBRINI
    30/11/2022, 11:20
  4. 3. Flavour anomalies 1
    Ulrik Egede (Monash University (AU))
    30/11/2022, 13:20
  5. 4. Flavour anomalies 2
    Ulrik Egede (Monash University (AU))
    30/11/2022, 14:20
  6. 5. Experimental techniques for dark matter detection
    Theresa Fruth
    30/11/2022, 15:50
  7. 8. Discussion
    30/11/2022, 16:50
  8. 9. Dark matter 3
    Yann MAMBRINI
    01/12/2022, 10:00
  9. 10. Flavour physics 3
    Ulrik Egede (Monash University (AU))
    01/12/2022, 11:20
  10. 11. Neutrino astrophysics 1
    Jenni Adams (University of Canterbury)
    01/12/2022, 13:20
  11. 12. Neutrino astrophysics 2
    Jenni Adams (University of Canterbury)
    01/12/2022, 14:20
  12. 13. Phenomenology of ultralight scalar dark matter
    Dr Yevgeny Stadnik (The University of Sydney)
    01/12/2022, 15:50
  13. 14. Discussion
    01/12/2022, 16:50
  14. 17. Neutrino astrophysics
    Jenni Adams (University of Canterbury)
    02/12/2022, 10:00
  15. 28. Primordial black holes
    Pippa Cole
    02/12/2022, 11:20
  16. 16. Axions
    Ciaran O'Hare (Sydney)
    02/12/2022, 13:20
  17. 22. Phenomenology of the companion-axion model
    02/12/2022, 14:20

    We study the phenomenology of the ‘companion-axion model’ consisting of two coupled QCD axions. The second axion is required to rescue the Peccei-Quinn solution to the strong-CP problem from the effects of colored gravitational instantons. We investigate here the combined phenomenology of axion-axion and axionphoton interactions, recasting present and future single-axion bounds onto the...

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  18. 23. Decaying warm dark matter
    02/12/2022, 14:40

    During the recent years, decaying dark matter models have received renewed interest as proposed solutions to the current cosmological tensions, mainly due to their flexible expansion histories and clustering properties. While much focus has been on decaying cold dark matter, in this talk, I will present our recent work on decaying warm dark matter based on our recent preprint arXiv:2205.13628....

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  19. 26. Sensitivity of Dark Matter-Nucleus Interactions to Nuclear Structure
    02/12/2022, 15:00

    Non-relativistic effective field theory (NREFT) is one approach used for describing the interaction of WIMPS with ordinary matter. Among other factors, these interactions are expected to be affected by the structure of the atomic nuclei in the target. The sensitivity of the nuclear response components of the WIMP-nucleus scattering amplitude is investigated using shell model calculations for...

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  20. 19. Stellar Probes of BSM Physics
    William DeRocco
    02/12/2022, 15:50
  21. 7. Pub dinner and drinks
    02/12/2022, 18:00
  22. 15. Cosmology 3
    Mikhail Shaposhnikov
  23. 18. Student talks
  24. 20. Student talks/discussion