Sydney Spring School 2022

Contribution List

6. Opening/Introductions

11/30/22, 9:45 AM

1. Dark matter 1

Yann MAMBRINI

11/30/22, 10:00 AM

2. Dark matter 2

Yann MAMBRINI

11/30/22, 11:20 AM

3. Flavour anomalies 1

Ulrik Egede (Monash University (AU))

11/30/22, 1:20 PM

4. Flavour anomalies 2

Ulrik Egede (Monash University (AU))

11/30/22, 2:20 PM

5. Experimental techniques for dark matter detection

Theresa Fruth

11/30/22, 3:50 PM

8. Discussion

11/30/22, 4:50 PM

9. Dark matter 3

Yann MAMBRINI

12/1/22, 10:00 AM

10. Flavour physics 3

Ulrik Egede (Monash University (AU))

12/1/22, 11:20 AM

11. Neutrino astrophysics 1

Jenni Adams (University of Canterbury)

12/1/22, 1:20 PM

12. Neutrino astrophysics 2

Jenni Adams (University of Canterbury)

12/1/22, 2:20 PM

13. Phenomenology of ultralight scalar dark matter

Dr Yevgeny Stadnik (The University of Sydney)

12/1/22, 3:50 PM

14. Discussion

12/1/22, 4:50 PM

17. Neutrino astrophysics

Jenni Adams (University of Canterbury)

12/2/22, 10:00 AM

28. Primordial black holes

Pippa Cole

12/2/22, 11:20 AM

16. Axions

Ciaran O'Hare (Sydney)

12/2/22, 1:20 PM

22. Phenomenology of the companion-axion model

12/2/22, 2:20 PM

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...

23. Decaying warm dark matter

12/2/22, 2:40 PM

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....

26. Sensitivity of Dark Matter-Nucleus Interactions to Nuclear Structure

12/2/22, 3:00 PM

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...

19. Stellar Probes of BSM Physics

William DeRocco

12/2/22, 3:50 PM

7. Pub dinner and drinks

12/2/22, 6:00 PM

15. Cosmology 3

Mikhail Shaposhnikov

18. Student talks

20. Student talks/discussion