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Axions in the Lab and in the Cosmos

15–19 Jul 2019
CERN
Europe/Zurich timezone

TH secretariat

Contribution List

17 out of 17 displayed
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  1. 7. Astro/cosmo probes of axions/ALPs
    Asimina Arvanitaki
    15/07/2019, 10:00
  2. 13. Discussion : Dynamical relaxation in a fuzzy dark matter halo
    Scott Tremaine
    15/07/2019, 13:30
  3. 1. Relic abundance of QCD axion DM
    Giovanni Villadoro
    15/07/2019, 15:00
  4. 14. Discussion: Relic abundance of axions
    Malte Buschmann (JGU Mainz)
    15/07/2019, 16:00
  5. 8. Higgs portal with an ALP
    Kwang Sik Jeong
    16/07/2019, 10:00
  6. 15. Discussion: ALP cosmology and its experimental implications
    Fuminobu Takahashi
    16/07/2019, 11:15
  7. 4. Overview of lab searches for axions
    Andreas Ringwald (Deutsches Elektronen-Synchrotron DESY)
    16/07/2019, 15:00
  8. 3. A model-building perspective on axion couplings
    Jihn E. Kim (Kyung Hee University)
    17/07/2019, 10:00
  9. 17. Discussion: Axion model-building
    Keisuke Harigaya (Institute for Advaned Study)
    17/07/2019, 11:00
  10. 2. Outstanding problems in axion cosmology
    David J. E. Marsh
    18/07/2019, 10:00
  11. 18. Discussion: Substructure in an axion dark matter halo — from vortices to black hole hair
    Lam Hui (Columbia University)
    18/07/2019, 13:30
  12. 6. The QCD axion at aLIGO
    Maria Baryakhtar
    19/07/2019, 10:00
  13. 12. Discussion: Astrophysical signatures of/bounds on axions
    Alessandro Mirizzi, Koichi Hamaguchi
    19/07/2019, 11:00
  14. 5. The Axion Echo method and the Big Flow
    Pierre Sikivie (University of Florida)
    19/07/2019, 15:00

    Electromagnetic radiation with angular frequency half the
    axion mass stimulates the decay of dark matter axions and
    produces an echo, i.e. faint electromagnetic radiation
    traveling in the opposite direction. Thus one may search
    for axion dark matter by sending out to space a powerful
    beam of electromagnetic radiation and listening for its
    echo. The method is particularly attractive if...

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  15. 9. Discussion: Dynamical relaxation in a fuzzy dark matter halo
    Scott Tremaine
  16. 10. Discussion: relic abundance of the QCD axion

    Discussion of recent achievements and open questions in the calculation of the relic abundance of the QCD axion, from misalignment to particle emission from strings to miniclusters.

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  17. 16. Test