FLASY 2024: the 10th Workshop on Flavor Symmetries and Consequences in Accelerators and Cosmology

Session

Flavor and Astrophysics

24 Jun 2024, 11:15

1010 (ISEB)

25. Adding Flavors to Axiogenesis and Spicing Up Cosmological Mysteries

Raymond Co (Indiana University)

24/06/2024, 11:15

A rotation in Peccei-Quinn field space along the axion direction can address cosmological mysteries, including dark matter, baryon asymmetry, cosmic perturbations, and the Hubble tension. This dynamics may naturally arise as a result of quantum gravity effects and cosmic inflation. Axion rotations can simultaneously give a new origin of axion dark matter via kinetic misalignment and generate...

29. Dark Matter Heating of Neutron Stars: Advantages and Challenges

Koichi Hamaguchi

24/06/2024, 15:15

Plenary Sessions

15. Flavoured Dark Matter - from Freeze-Out Scenarios to LHC Signatures

Monika Blanke (Karlsruhe Institute of Technology)

25/06/2024, 09:15

Plenary Sessions

23. Flavorful Dark Matter

Xiao-Gang He

25/06/2024, 10:30

30. Searching for light accelerated dark matter

Gopolang Mohlabeng (University of California, Irvine)

25/06/2024, 11:15

Low mass accelerated dark matter (DM) is very well motivated and has been a subject of much attention in the literature. These fast-moving particles can gain enough kinetic energy to surpass the energy thresholds of some Large volume terrestrial detectors. For instance, fast-moving DM can deposit sizable amounts of energy at both large volume neutrino detectors and dark matter direct detection...

28. Flavonic dark matter

Eung Jin Chun

25/06/2024, 14:00

We present a common solution to dark matter and the flavor problem n the framework of the discrete flavor symmetry.

where the associated flavonic Goldstone boson acts as a good dark matter candidate through the misalignment mechanism.

For light active neutrinos, the Dirac-type mass matrix is preferred to fit the observed neutrino oscillation data with normal hierarchy.

Our model...

5. An axion-like particle explanation of $B\to \pi K$ puzzle and $B \to K \nu \bar{\nu} $ excess

Shibasis Roy

Parallel Sessions

2. Flavor Physics in the Dark Sector

LINGFENG LI (Brown U.)

Parallel Sessions

38. Searching for light accelerated dark matter

Gopolang Mohlabeng (Simon Fraser University)

Plenary Sessions