Numerical method for binary black hole/neutron star initial data: Code test

2007 ◽  
Vol 75 (4) ◽  
Author(s):  
Antonios A. Tsokaros ◽  
Kōji Uryū
2007 ◽  
Vol 76 (10) ◽  
Author(s):  
Zachariah B. Etienne ◽  
Joshua A. Faber ◽  
Yuk Tung Liu ◽  
Stuart L. Shapiro ◽  
Thomas W. Baumgarte

2015 ◽  
Vol 32 (24) ◽  
pp. 245010 ◽  
Author(s):  
Serguei Ossokine ◽  
Francois Foucart ◽  
Harald P Pfeiffer ◽  
Michael Boyle ◽  
Béla Szilágyi

2016 ◽  
Vol 93 (4) ◽  
Author(s):  
Kevin Barkett ◽  
Mark A. Scheel ◽  
Roland Haas ◽  
Christian D. Ott ◽  
Sebastiano Bernuzzi ◽  
...  

Author(s):  
Sarah Habib ◽  
Antoni Ramos-Buades ◽  
Eliu Huerta ◽  
Sascha Husa ◽  
Roland Haas ◽  
...  

2013 ◽  
pp. 394-428
Author(s):  
Thomas W. Baumgarte ◽  
Stuart L. Shapiro

2005 ◽  
Vol 02 (02) ◽  
pp. 497-520 ◽  
Author(s):  
HARALD P. PFEIFFER

The conformal method for constructing initial data for Einstein's equations is presented in both the Hamiltonian and Lagrangian picture (extrinsic curvature decomposition and conformal thin sandwich formalism, respectively), and advantages due to the recent introduction of a weight-function in the extrinsic curvature decomposition are discussed. I then describe recent progress in numerical techniques to solve the resulting elliptic equations, and explore innovative approaches toward the construction of astrophysically realistic initial data for binary black hole simulations.


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