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The SXS Collaboration's third catalog of binary black hole simulations

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Scheel, Mark A., Boyle, Michael, Mitman, Keefe, Deppe, Nils, Stein, Leo C., Armaza, Cristóbal, Bonilla, Marceline S., Buchman, Luisa T., Ceja, Andrea, Chaudhary, Himanshu, Chen, Yitian, Corman, Maxence, Csukás, Károly Zoltán, Ferrus, C. Melize, Field, Scott E., Giesler, Matthew, Habib, Sarah, Hébert, François, Hemberger, Daniel A., Iozzo, Dante A. B., Islam, Tousif, Jones, Ken Z., Khairnar, Aniket, Kidder, Lawrence E., Knapp, Taylor, Kumar, Prayush, Lara, Guillermo, Long, Oliver, Lovelace, Geoffrey, Ma, Sizheng, Melchor, Denyz, Morales, Marlo, Moxon, Jordan, Nee, Peter James, Nelli, Kyle C., O'Shea, Eamonn, Ossokine, Serguei, Owen, Robert, Pfeiffer, Harald P., Pretto, Isabella G., Ramirez-Aguilar, Teresita, Ramos-Buades, Antoni, Ravichandran, Adhrit, Ravishankar, Abhishek, Rodriguez, Samuel, Rüter, Hannes R., Sanchez, Jennifer, Shaikh, Md Arif, Sun, Dongze, Szilágyi, Béla, Tellez, Daniel, Teukolsky, Saul A., Thomas, Sierra, Throwe, William, Varma, Vijay, Vu, Nils L., Walker, Marissa, Wittek, Nikolas A., Yoo, Jooheon
Format:	Preprint
Publié:	2025
Sujets:	General Relativity and Quantum Cosmology
Accès en ligne:	Acceder al recurso
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_version_	1866911198085120000
author	Scheel, Mark A. Boyle, Michael Mitman, Keefe Deppe, Nils Stein, Leo C. Armaza, Cristóbal Bonilla, Marceline S. Buchman, Luisa T. Ceja, Andrea Chaudhary, Himanshu Chen, Yitian Corman, Maxence Csukás, Károly Zoltán Ferrus, C. Melize Field, Scott E. Giesler, Matthew Habib, Sarah Hébert, François Hemberger, Daniel A. Iozzo, Dante A. B. Islam, Tousif Jones, Ken Z. Khairnar, Aniket Kidder, Lawrence E. Knapp, Taylor Kumar, Prayush Lara, Guillermo Long, Oliver Lovelace, Geoffrey Ma, Sizheng Melchor, Denyz Morales, Marlo Moxon, Jordan Nee, Peter James Nelli, Kyle C. O'Shea, Eamonn Ossokine, Serguei Owen, Robert Pfeiffer, Harald P. Pretto, Isabella G. Ramirez-Aguilar, Teresita Ramos-Buades, Antoni Ravichandran, Adhrit Ravishankar, Abhishek Rodriguez, Samuel Rüter, Hannes R. Sanchez, Jennifer Shaikh, Md Arif Sun, Dongze Szilágyi, Béla Tellez, Daniel Teukolsky, Saul A. Thomas, Sierra Throwe, William Varma, Vijay Vu, Nils L. Walker, Marissa Wittek, Nikolas A. Yoo, Jooheon
author_facet	Scheel, Mark A. Boyle, Michael Mitman, Keefe Deppe, Nils Stein, Leo C. Armaza, Cristóbal Bonilla, Marceline S. Buchman, Luisa T. Ceja, Andrea Chaudhary, Himanshu Chen, Yitian Corman, Maxence Csukás, Károly Zoltán Ferrus, C. Melize Field, Scott E. Giesler, Matthew Habib, Sarah Hébert, François Hemberger, Daniel A. Iozzo, Dante A. B. Islam, Tousif Jones, Ken Z. Khairnar, Aniket Kidder, Lawrence E. Knapp, Taylor Kumar, Prayush Lara, Guillermo Long, Oliver Lovelace, Geoffrey Ma, Sizheng Melchor, Denyz Morales, Marlo Moxon, Jordan Nee, Peter James Nelli, Kyle C. O'Shea, Eamonn Ossokine, Serguei Owen, Robert Pfeiffer, Harald P. Pretto, Isabella G. Ramirez-Aguilar, Teresita Ramos-Buades, Antoni Ravichandran, Adhrit Ravishankar, Abhishek Rodriguez, Samuel Rüter, Hannes R. Sanchez, Jennifer Shaikh, Md Arif Sun, Dongze Szilágyi, Béla Tellez, Daniel Teukolsky, Saul A. Thomas, Sierra Throwe, William Varma, Vijay Vu, Nils L. Walker, Marissa Wittek, Nikolas A. Yoo, Jooheon
contents	We present a major update to the Simulating eXtreme Spacetimes (SXS) Collaboration's catalog of binary black hole simulations. Using highly efficient spectral methods implemented in the Spectral Einstein Code (SpEC), we have nearly doubled the total number of binary configurations from 2,018 to 3,756. The catalog now densely covers the parameter space with precessing simulations up to mass ratio $q=8$ and dimensionless spins up to $\|\vecχ\|\le0.8$ with near-zero eccentricity. The catalog also includes some simulations at higher mass ratios with moderate spin and more than 250 eccentric simulations. We have also deprecated and rerun some simulations from our previous catalog (e.g., simulations run with a much older version of SpEC or that had anomalously high errors in the waveform). The median waveform difference (which is similar to the mismatch) between resolutions over the simulations in the catalog is $4\times10^{-4}$. The simulations have a median of 22 orbits, while the longest simulation has 148 orbits. We have corrected each waveform in the catalog to be in the binary's center-of-mass frame and exhibit gravitational-wave memory. We estimate the total CPU cost of all simulations in the catalog to be 480,000,000 core-hours. We find that using spectral methods for binary black hole simulations is over 1,000 times more efficient than much shorter finite-difference simulations of comparable accuracy. The full catalog is publicly available through the sxs Python package and at https://data.black-holes.org .
format	Preprint
id	arxiv_https___arxiv_org_abs_2505_13378
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	The SXS Collaboration's third catalog of binary black hole simulations Scheel, Mark A. Boyle, Michael Mitman, Keefe Deppe, Nils Stein, Leo C. Armaza, Cristóbal Bonilla, Marceline S. Buchman, Luisa T. Ceja, Andrea Chaudhary, Himanshu Chen, Yitian Corman, Maxence Csukás, Károly Zoltán Ferrus, C. Melize Field, Scott E. Giesler, Matthew Habib, Sarah Hébert, François Hemberger, Daniel A. Iozzo, Dante A. B. Islam, Tousif Jones, Ken Z. Khairnar, Aniket Kidder, Lawrence E. Knapp, Taylor Kumar, Prayush Lara, Guillermo Long, Oliver Lovelace, Geoffrey Ma, Sizheng Melchor, Denyz Morales, Marlo Moxon, Jordan Nee, Peter James Nelli, Kyle C. O'Shea, Eamonn Ossokine, Serguei Owen, Robert Pfeiffer, Harald P. Pretto, Isabella G. Ramirez-Aguilar, Teresita Ramos-Buades, Antoni Ravichandran, Adhrit Ravishankar, Abhishek Rodriguez, Samuel Rüter, Hannes R. Sanchez, Jennifer Shaikh, Md Arif Sun, Dongze Szilágyi, Béla Tellez, Daniel Teukolsky, Saul A. Thomas, Sierra Throwe, William Varma, Vijay Vu, Nils L. Walker, Marissa Wittek, Nikolas A. Yoo, Jooheon General Relativity and Quantum Cosmology We present a major update to the Simulating eXtreme Spacetimes (SXS) Collaboration's catalog of binary black hole simulations. Using highly efficient spectral methods implemented in the Spectral Einstein Code (SpEC), we have nearly doubled the total number of binary configurations from 2,018 to 3,756. The catalog now densely covers the parameter space with precessing simulations up to mass ratio $q=8$ and dimensionless spins up to $\|\vecχ\|\le0.8$ with near-zero eccentricity. The catalog also includes some simulations at higher mass ratios with moderate spin and more than 250 eccentric simulations. We have also deprecated and rerun some simulations from our previous catalog (e.g., simulations run with a much older version of SpEC or that had anomalously high errors in the waveform). The median waveform difference (which is similar to the mismatch) between resolutions over the simulations in the catalog is $4\times10^{-4}$. The simulations have a median of 22 orbits, while the longest simulation has 148 orbits. We have corrected each waveform in the catalog to be in the binary's center-of-mass frame and exhibit gravitational-wave memory. We estimate the total CPU cost of all simulations in the catalog to be 480,000,000 core-hours. We find that using spectral methods for binary black hole simulations is over 1,000 times more efficient than much shorter finite-difference simulations of comparable accuracy. The full catalog is publicly available through the sxs Python package and at https://data.black-holes.org .
title	The SXS Collaboration's third catalog of binary black hole simulations
topic	General Relativity and Quantum Cosmology
url	https://arxiv.org/abs/2505.13378