20–22 Jul 2020
Europe/Zurich timezone

Session

Online talk

20 Jul 2020, 15:00

Conveners

Online talk: Opening talk

  • Florian Reindl (HEPHY & TU Vienna)

Online talk: Direct detection I

  • Florian Reindl (HEPHY & TU Vienna)

Online talk: Direct detection II

  • Valentyna Mokina (HEPHY)

Online talk: Direct detection III

  • Josef Pradler (Austrian Academy of Sciences (AT))

Online talk: Bound-state DM

  • Josef Pradler (Austrian Academy of Sciences (AT))

Online talk: Cosmology and DM simulations

  • Holger Kluck (HEPHY)

Online talk: Axion DM

  • Holger Kluck (HEPHY)

Online talk: Sterile neutrinos

  • Jochen Schieck (Austrian Academy of Sciences (AT))

Online talk: Indirect detection and accelerator searches

  • Jochen Schieck (Austrian Academy of Sciences (AT))

Online talk: Accelerator searches and indirect detection

  • Anastasia Sokolenko (HEPHY)

Presentation materials

There are no materials yet.

  1. Kathryn Mary Zurek (University of California Berkeley (US))
    20/07/2020, 15:00
    Oral presentation
  2. Richard Gaitskell (Brown University)
    20/07/2020, 15:30
    Oral presentation
  3. Jodi Cooley (SMU)
    20/07/2020, 16:00
    Oral presentation
  4. Carla Macolino (LAL/CNRS)
    20/07/2020, 16:45
    Oral presentation
  5. Elisabetta Baracchini (Gran Sasso Science Institute)
    20/07/2020, 17:15
    Oral presentation
  6. Felix Kahlhoefer (RWTH Aachen)
    20/07/2020, 17:45
    Oral presentation
  7. Rouven Essig
    21/07/2020, 15:00
    Oral presentation
  8. Gordan Krnjaic (Fermilab)
    21/07/2020, 15:30
    Oral presentation
  9. Juri Smirnov (Ohio State University)
    21/07/2020, 16:00
    Oral presentation
  10. Dr Katie Mack (North Carolina State University)
    21/07/2020, 16:45
    Oral presentation
  11. Carlos Frenk (University of Durham)
    21/07/2020, 17:15
    Oral presentation
  12. Dr Luca Visinelli (GRAPPA, University of Amsterdam)
    21/07/2020, 17:45
    Oral presentation

    Axions and axion-like particles are excellent dark matter candidates, spanning a vast range of mass scales from the milli- and micro-eV for the QCD axion, to 10^(-22)eV for ultralight axions that make up the "axiverse". In some scenarios, the collapse of the non-homogeneous axion field leads to the formation of two kind of compact structures, known as axion "miniclusters" and axion "stars". I...

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  13. Karl van Bibber (University of California Berkeley)
    21/07/2020, 18:15
    Oral presentation
  14. Prof. Oleg Ruchayskiy (University of Copenhagen (DK))
    22/07/2020, 15:00
    Oral presentation
  15. Alexey Boyarsky (Leiden University (NL))
    22/07/2020, 15:30
    Oral presentation
  16. Rebecca Leane (Massachusetts Institute of Technology)
    22/07/2020, 16:00
    Oral presentation
  17. Chang-Seong Moon (Kyungpook National University (KR))
    22/07/2020, 16:30
    Oral presentation
  18. Enrico Graziani (INFN - National Institute for Nuclear Physics)
    22/07/2020, 17:15
    Oral presentation
  19. Tim Linden
    22/07/2020, 17:45
    Oral presentation
  20. Tracy Slatyer
    22/07/2020, 18:15
    Oral presentation
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