- "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, March 13, Hector Iglesias, UT Austin, Hybridization of WaSABI-C inspirals with numerical relativity waveforms for quasi-circular, spin-aligned, asymmetric black hole binaries
370 Cahill & Zoom: 851 0756 7442
ARC Seminars
TAPIR also hosts ARC Seminars Tuesdays at 3:00pm in 319 Cahill