"Race tracks" followed by a pair of two unequal mass black holes with misaligned spins. The orbits are precessing. The two black holes have formed a common horizon, which is shown as a third surface around the two individucal horizons. (SXS Collaboration, learn more)
- "Race tracks" followed by a pair of two unequal mass black holes with misaligned spins. The orbits are precessing. The two black holes have formed a common horizon, which is shown as a third surface around the two individucal horizons. (SXS Collaboration, learn more)
TAPIR is part of the Division of Physics, Mathematics, and Astronomy at Caltech. We are located in the Cahill Center for Astronomy and Astrophysics.
TAPIR Seminars
The next TAPIR Seminar will be Friday, May 3, Alex Vañó-Viñuales, Univ of Lisbon,
Current numerical efforts on free hyperboloidal evolutions
370 Cahill and Zoom: 868 5298 8404