About
Binary black holes are the most numerous source of observed gravitational waves (GW). Precise knowledge about the interaction between two black holes and the emitted GWs are of high importance for finding and analysing GW signals, as well as to deepen the understanding of the structure and solutions of Einstein's equations. In this talk, I summarize the contributions of Numerical Relativity simulations to GW astrophysics, touching on all types of orbits (quasi-circular, eccentric, hyperbolic). Emphasis will be on results obtained with the SpEC code of the SXS collaboration..
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The talk
Credits and licence
- Institution
- CERN
- Department
- Conferences, Workshops & Schools
- Speaker
- Harald Pfeiffer
- Year
- 2023
- Language
- English
- Source
- CERN
- Licence
- CERN, as CERN states it. CERN's terms
- Attribution
- © CERN. CERN provides its audiovisual media free of charge for educational and informational use, credited to CERN; this lecture is shown in CERN's own player.
- Who can watch
- CERN gives no rating. Invisible Network shows it to Teens profiles and older, judged from what the source says about it. How courses are placed