23–26 Mar 2026
Europe/London timezone

Contribution List

27 out of 27 displayed
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  1. Jack Shergold
    23/03/2026, 14:00
  2. Tetiana Kozynets
    23/03/2026, 14:45
  3. Sergey Burdin
    23/03/2026, 16:00
  4. M. Sten Delos
    24/03/2026, 09:30

    I will present prompt cusps, a recently identified class of compact dark matter structures with ρ∝r^-1.5 density profiles that form at the onset of structure formation and persist at halo centers. These systems enable new constraints on warm dark matter from dwarf galaxy kinematics, strengthen limits on annihilating dark matter, and offer detection prospects for general cold dark matter...

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  5. Yann Gouttenoire
    24/03/2026, 10:15

    Explaining the large amplitude of the nano-Hertz stochastic gravitational-wave background observed by pulsar timing arrays (PTAs) typically requires extremely energetic primordial sources. Such mechanisms generically produce large curvature perturbations, which subsequently collapse into ultra-compact mini-halos (UCMHs). If
    dark matter consists of weakly interacting massive particles...

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  6. Tanmay Poddar
    24/03/2026, 11:30
  7. 24/03/2026, 13:45
  8. Martin Bauer
    24/03/2026, 14:30
  9. Spencer Griffith
    24/03/2026, 15:45
  10. Ed Daw
    24/03/2026, 16:30
  11. Fatemeh Elahi
    25/03/2026, 09:30
  12. Malcolm Fairbairn
    25/03/2026, 10:45
  13. Henry Stubbs
    25/03/2026, 11:30

    Nearly 30 years since the ADD proposal to solve the hierarchy problem via large extra dimensions, such scenarios have seen a resurgence in interest in the context of the ‘dark dimension’ - an extra dimension of micron scale motivated by the swampland program. We will begin by reviewing the features of the dark dimension, including the possibility that dark matter could consist of Kaluza-Klein...

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  14. Anne Green
    25/03/2026, 13:45
  15. Miguel Crispim Romao
    25/03/2026, 14:30
  16. 25/03/2026, 15:15
  17. 25/03/2026, 19:00
  18. Ashlea Kemp
    26/03/2026, 09:15
  19. Keir Rogers
    26/03/2026, 10:00

    The fundamental nature of dark matter so far eludes direct detection experiments, but it has left its imprint in the cosmic large-scale structure. Disentangling this imprint requires accurate modelling of structure formation in non-standard dark matter models, careful handling of astrophysical uncertainties and consistent observations in independent cosmological probes. I will review a...

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  20. Jocelyn Monroe
    26/03/2026, 11:15
  21. Sukannya Bhattacharya