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GR: Fachverband Gravitation, Relativistische Astrophysik und Kosmologie
GR 3: Classical General Relativity I
Montag, 16. März 2026, 16:15–17:30, KH 02.012
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16:15 | GR 3.1 | What can Holography teach us about scale without conformal invariance? — •Lavish Chawla and Mario Flory |
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16:30 | GR 3.2 | Formulating the complete initial boundary value problem in numerical relativity to model black hole echoes — •Conner Dailey |
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16:45 | GR 3.3 | Revisiting Synchronisation Systems and Applications in Geodesy — •Bennet Grützner, Eva Hackmann, and Claus Lämmerzahl |
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17:00 | GR 3.4 | Discrete Spacetime Blocks for Visualizing GR: Interactive Geodesics in a (2+1D) Schwarzschild Sector Model — •Vassilios Marakis, Rahel Gabriel, Corvin Zahn, and Ute Kraus |
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17:15 | GR 3.5 | Relativistic orbital perturbation theory — Oleksii Yanchyshen, Eva Hackmann, and •Claus Lämmerzahl |