scholarly journals Inferring black-hole orbital dynamics from numerical-relativity gravitational waveforms

2018 ◽  
Vol 98 (8) ◽  
Author(s):  
Eleanor Hamilton ◽  
Mark Hannam
2020 ◽  
Vol 102 (4) ◽  
Author(s):  
Andrew Matas ◽  
Tim Dietrich ◽  
Alessandra Buonanno ◽  
Tanja Hinderer ◽  
Michael Pürrer ◽  
...  

2019 ◽  
Vol 69 (1) ◽  
pp. 41-64 ◽  
Author(s):  
Masaru Shibata ◽  
Kenta Hotokezaka

Mergers of binary neutron stars and black hole–neutron star binaries are among the most promising sources for ground-based gravitational-wave (GW) detectors and are also high-energy astrophysical phenomena, as illustrated by the observations of GWs and electromagnetic (EM) waves in the event of GW170817. Mergers of these neutron star binaries are also the most promising sites for r-process nucleosynthesis. Numerical simulation in full general relativity (numerical relativity) is a unique approach to the theoretical prediction of the merger process, GWs emitted, mass ejection process, and resulting EM emission. We summarize the current understanding of the processes of neutron star mergers and subsequent mass ejection based on the results of the latest numerical-relativity simulations. We emphasize that the predictions of the numerical-relativity simulations agree broadly with the optical and IR observations of GW170817.


2019 ◽  
Vol 99 (8) ◽  
Author(s):  
Robert Owen ◽  
Alex S. Fox ◽  
John A. Freiberg ◽  
Terrence Pierre Jacques

2010 ◽  
Vol 104 (21) ◽  
Author(s):  
Carlos O. Lousto ◽  
Hiroyuki Nakano ◽  
Yosef Zlochower ◽  
Manuela Campanelli

2016 ◽  
Vol 25 (09) ◽  
pp. 1641022 ◽  
Author(s):  
Emanuele Berti ◽  
Vitor Cardoso ◽  
Luis C. B. Crispino ◽  
Leonardo Gualtieri ◽  
Carlos Herdeiro ◽  
...  

We review recent progress in the application of numerical relativity techniques to astrophysics and high-energy physics. We focus on recent developments regarding the spin evolution in black hole binaries, high-energy black hole collisions, compact object solutions in scalar–tensor gravity, superradiant instabilities, hairy black hole solutions in Einstein’s gravity coupled to fundamental fields, and the possibility to gain insight into these phenomena using analog gravity models.


2013 ◽  
Vol 88 (12) ◽  
Author(s):  
Alexandre Le Tiec ◽  
Alessandra Buonanno ◽  
Abdul H. Mroué ◽  
Harald P. Pfeiffer ◽  
Daniel A. Hemberger ◽  
...  

2015 ◽  
Vol 115 (12) ◽  
Author(s):  
Jonathan Blackman ◽  
Scott E. Field ◽  
Chad R. Galley ◽  
Béla Szilágyi ◽  
Mark A. Scheel ◽  
...  

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