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UTC
    • 08:30 08:50
      Registration & Coffee 20m
    • 08:50 09:00
      Opening Remarks 10m
    • 09:00 10:00
      LIGO I 1h
      We perform scalar self-force calculations for inclined, eccentric orbits of a small, compact body in Kerr spacetime. To implement these calculations with arbitrary numerical precision, we generalize spectral source integration (SSI) techniques by introducing the Mino time parameter and extending mode decompositions to include a polar frequency for inclined motion. Calculations are conducted using a Mathematica code that implements these SSI techniques along with the Mano, Suzuki, and Takasugi (MST) formalism to determine the inhomogeneous wave function solutions to the Teukolsky equation. This allows us to improve the accuracy of previous calculations in the literature. We also probe the extended parameter space for various orbital inclinations. Further extension to the gravitational case is also considered.
      Speaker: Aaron Zimmerman
      Slides
    • 10:00 11:00
      LIGO II 1h
      Speaker: Jonathan Gair
    • 11:00 11:30
      Break 30m
    • 11:30 12:00
      Talk 1 30m
    • 12:00 12:30
      Talk 2 30m
    • 12:30 14:00
      Lunch 1h 30m
    • 14:00 14:30
      Talk 3 30m
    • 14:30 15:00
      Talk 4 30m
    • 15:00 15:30
      Talk 5 30m
    • 15:30 16:00
      Break 30m
    • 16:00 16:30
      Talk 6 30m
    • 16:30 17:00
      Talk 7 30m
    • 17:00 18:00
      Open Discussion 1h
    • 09:00 10:00
      Self-Force Evolution 1h
      Speaker: Niels Warburton
    • 10:00 11:00
      Self-Force Kerr 1h
      Speaker: Maarten van de Meent
    • 09:00 10:00
      Second-Order 1h
      Speaker: Adam Pound
    • 10:00 11:00
      Effective Source 1h
      Speaker: Barry Wardell
    • 09:00 10:00
      Laws of Binary Black Holes 1h
      Speaker: Alexandre Le Tiec
    • 10:00 11:00
      EOB I 1h
      Speaker: Alessandro Taracchini
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