"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 Seminar
The next TAPIR Seminar will be Friday, September 29, Monica Gallegos-Garcia, Northwestern Univ,
Gaining Physical Insights into the Formation of Black-Hole Mergers
Hybrid - Join via Zoom: 864 8902 5566