The SXS collaboration catalog of binary black hole simulations

Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximum science. Near the time of merger, the gravitational waves from merging black holes can be computed only using numerical relativity. In this p...

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Veröffentlicht in:	Classical and quantum gravity 2019-10, Vol.36 (19), p.195006
Hauptverfasser:	Boyle, Michael, Hemberger, Daniel, Iozzo, Dante A B, Lovelace, Geoffrey, Ossokine, Serguei, Pfeiffer, Harald P, Scheel, Mark A, Stein, Leo C, Woodford, Charles J, Zimmerman, Aaron B, Afshari, Nousha, Barkett, Kevin, Blackman, Jonathan, Chatziioannou, Katerina, Chu, Tony, Demos, Nicholas, Deppe, Nils, Field, Scott E, Fischer, Nils L, Foley, Evan, Fong, Heather, Garcia, Alyssa, Giesler, Matthew, Hebert, Francois, Hinder, Ian, Katebi, Reza, Khan, Haroon, Kidder, Lawrence E, Kumar, Prayush, Kuper, Kevin, Lim, Halston, Okounkova, Maria, Ramirez, Teresita, Rodriguez, Samuel, Rüter, Hannes R, Schmidt, Patricia, Szilagyi, Bela, Teukolsky, Saul A, Varma, Vijay, Walker, Marissa
Format:	Artikel
Sprache:	eng
Schlagworte:	black holes gravitational waves numerical relativity
Online-Zugang:	Volltext
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