F
Francois Hebert
Researcher at California Institute of Technology
Publications - 26
Citations - 630
Francois Hebert is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Gravitational wave & Numerical relativity. The author has an hindex of 7, co-authored 19 publications receiving 368 citations. Previous affiliations of Francois Hebert include Cornell University.
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Journal ArticleDOI
The SXS collaboration catalog of binary black hole simulations
Michael Boyle,Daniel A. Hemberger,Dante A. B. Iozzo,Geoffrey Lovelace,Geoffrey Lovelace,Serguei Ossokine,Harald P. Pfeiffer,Mark A. Scheel,Leo C. Stein,Leo C. Stein,Charles J. Woodford,Aaron Zimmerman,Nousha Afshari,Kevin Barkett,Jonathan Blackman,Katerina Chatziioannou,Tony Chu,Nicholas Demos,Nils Deppe,Scott E. Field,Scott E. Field,Nils Fischer,E. Foley,Heather Fong,Heather Fong,Alyssa Garcia,Matthew Giesler,Francois Hebert,Ian Hinder,Ian Hinder,Reza Katebi,H. Khan,Lawrence E. Kidder,Prayush Kumar,Prayush Kumar,Kevin Kuper,Halston Lim,Halston Lim,Maria Okounkova,T. D. Ramirez,S. Rodriguez,Hannes R. Rüter,Patricia Schmidt,Patricia Schmidt,Béla Szilágyi,Saul A. Teukolsky,Saul A. Teukolsky,Vijay Varma,Michelle E. Walker +48 more
TL;DR: In this paper, a major update of the Simulating eXtreme Spacetimes (SXS) Collaboration catalog of numerical simulations for merging black holes is presented, including 1426 spin-precessing configurations with mass ratios between 1 and 10, and spin magnitudes up to 0.998.
Journal ArticleDOI
What does a binary black hole merger look like
Andy Bohn,William Throwe,Francois Hebert,Katherine Henriksson,Darius Bunandar,Nicholas Taylor,Mark A. Scheel +6 more
TL;DR: In this paper, a method of calculating the strong-field gravitational lensing caused by many analytic and numerical spacetimes is presented, which is used to calculate the distortion caused by isolated black holes and by numerically evolved black hole binaries.
Journal ArticleDOI
What does a binary black hole merger look like
Andy Bohn,William Throwe,Francois Hebert,Katherine Henriksson,Darius Bunandar,Darius Bunandar,Mark A. Scheel,Nicholas Taylor +7 more
TL;DR: In this article, a method of calculating the strong-field gravitational lensing caused by many analytic and numerical spacetimes is presented, which is used to calculate the distortion caused by isolated black holes (BHs) and by numerically evolved BH binaries.
Journal ArticleDOI
SpECTRE: A task-based discontinuous Galerkin code for relativistic astrophysics
Lawrence E. Kidder,Scott E. Field,Scott E. Field,Francois Foucart,Erik Schnetter,Erik Schnetter,Erik Schnetter,Saul A. Teukolsky,Andy Bohn,Nils Deppe,Peter Diener,Francois Hebert,Jonas Lippuner,Jonah Miller,Jonah Miller,Christian D. Ott,Mark A. Scheel,Trevor Vincent +17 more
TL;DR: SpECTRE as mentioned in this paper combines a discontinuous Galerkin method with a task-based parallelism model to achieve more accurate solutions for challenging relativistic astrophysics problems such as corecollapse supernovae and binary neutron star mergers.
Journal ArticleDOI
The SXS Collaboration catalog of binary black hole simulations
Michael Boyle,Daniel A. Hemberger,Dante A. B. Iozzo,Geoffrey Lovelace,Geoffrey Lovelace,Serguei Ossokine,Harald P. Pfeiffer,Mark A. Scheel,Leo C. Stein,Leo C. Stein,Charles J. Woodford,Aaron Zimmerman,Nousha Afshari,Kevin Barkett,Jonathan Blackman,Katerina Chatziioannou,Tony Chu,Nicholas Demos,Nils Deppe,Scott E. Field,Scott E. Field,Nils Fischer,E. Foley,Heather Fong,Heather Fong,Alyssa Garcia,Matthew Giesler,Francois Hebert,Ian Hinder,Ian Hinder,Reza Katebi,H. Khan,Lawrence E. Kidder,Prayush Kumar,Prayush Kumar,Kevin Kuper,Halston Lim,Halston Lim,Maria Okounkova,T. D. Ramirez,S. Rodriguez,Hannes R. Rüter,Patricia Schmidt,Patricia Schmidt,Béla Szilágyi,Saul A. Teukolsky,Saul A. Teukolsky,Vijay Varma,Michelle E. Walker +48 more
TL;DR: A major update of the Simulating eXtreme Spacetimes (SXS) Collaboration catalog of numerical simulations for merging black holes is presented in this paper, including 1426 spin-precessing configurations, with mass ratios between 1 and 10, and spin magnitudes up to 0.998.