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Gravitational Waves Beyond the Boxes II

Apr 4 – 8, 2022
Perimeter Institute for Theoretical Physics
America/Toronto timezone

Stephanie Mohl

Contribution List

18 out of 18 displayed
  1. 1. Welcome and Opening Remarks
    Daniel Siegel (Perimeter Institute & University of Guelph), Huan Yang (Perimeter Institute & University of Guelph), Luis Lehner (Perimeter Institute), Reed Essick (Perimeter Institute), Suvodip Mukherjee (Perimeter Institute), William East (Perimeter Institute)
    4/4/22, 8:50 AM
  2. 2. Measure the cosmic expansion history of the Universe using GW sources
    Jonathan Gair (Max Planck Institute for Gravitational Physics)
    4/4/22, 9:00 AM
  3. 3. Cross-correlation technique in GW cosmology
    Benjamin Wandelt (Institut d’Astrophysique de Paris)
    4/4/22, 10:00 AM
  4. 5. Matter in Extreme Conditions
    Katerina Chatziioannou (California Institute of Technology)
    4/4/22, 1:15 PM
  5. 9. Matter Effects in Waveform Models
    Geraint Pratten (University of Birmingham)
    4/5/22, 9:00 AM
  6. 7. Dark matter, PBHs, boson clouds
    Salvatore Vitale (Massachusetts Institute of Technology)
    4/5/22, 10:00 AM
  7. 8. Multi-band GW observation from the third-generation detectors - presented virtually
    Hsin-Yu Chen (Massachusetts Institute of Technology)
    4/5/22, 1:15 PM
  8. 6. Pulsar Timing Arrays - presented virtually
    Xavier Siemens (Oregon State University)
    4/5/22, 2:15 PM
  9. 10. Astrophysical populations and waveform models to test fundamental physics
    Maximiliano Isi (Flatiron Institute)
    4/6/22, 9:00 AM
  10. 11. Astrophysical populations and waveform modelling challenges to study cosmology
    Maya Fishbach (Northwestern University)
    4/6/22, 10:00 AM
  11. 12. Gravitational-wave observations of compact binary mergers
    Patricia Schmidt (University of Birmingham)
    4/6/22, 2:00 PM

    The first direct detection of gravitational waves from merging black holes in 2015 has opened up new avenues to studying gravity in the strong-field regime, inferring the mass and spin distributions of astrophysical black holes and probing the nature of ultra-dense nuclear matter in the interior of neutron stars. Seven years on, we count approximately 100 detections of gravitational waves from...

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  12. 13. Astrophysical stochastic background
    Thomas Callister (Flatiron Institute)
    4/7/22, 9:00 AM
  13. 14. Cosmological stochastic background - presented virtually
    Raphael Flauger (University of California, San Diego)
    4/7/22, 10:00 AM
  14. 15. Analytic waveform models
    Riccardo Sturani (ICTP SAIFR)
    4/7/22, 1:15 PM
  15. 17. Modeling waveform uncertainty - presented virtually
    Michael Pürrer (Max Planck Institute for Gravitational Physics)
    4/8/22, 9:00 AM
  16. 18. Closing Remarks
    Daniel Siegel (Perimeter Institute & University of Guelph), Huan Yang (Perimeter Institute & University of Guelph), Luis Lehner (Perimeter Institute), Reed Essick (Perimeter Institute), Suvodip Mukherjee (Perimeter Institute), William East (Perimeter Institute)
    4/8/22, 12:30 PM
  17. 16. Discussion Session: The impact of detector calibration
  18. 4. Tests of fundamental physics in both the strong and weak-field regimes - presented virtually
    Michalis Agathos (University of Cambridge)