2025-10-08 カリフォルニア工科大学（Caltech）
Web要約 の発言：
In this still from a binary black hole simulation, the upper half shows the horizons and past trajectories of the two black holes. The bottom half shows the space-time geometry in the orbital plane of the binary. The depth of the surface is proportional to the rate of time flow with redder colors representing slower time flows; the arrows show the velocity of the flow of space.
＜関連情報＞
- https://www.caltech.edu/about/news/catalog-of-simulations-of-black-hole-collisions-expands
- https://iopscience.iop.org/article/10.1088/1361-6382/adfd34
SXS共同研究による連星ブラックホールシミュレーションの第3カタログ The SXS collaboration’s third catalog of binary black hole simulations
Mark A Scheel, Michael Boyle, Keefe Mitman, Nils Deppe, Leo C Stein, Cristóbal Armaza, Marceline S Bonilla, Luisa T Buchman, Andrea Ceja, Himanshu Chaudhary,…
Classical and Quantum Gravity Published: 6 October 2025
DOI:10.1088/1361-6382/adfd34
Abstract
We present a major update to the Simulating eXtreme Spacetimes (SXSs) Collaboration’s catalog of binary black hole (BBH) simulations. Using highly efficient spectral methods implemented in the Spectral Einstein Code (SpEC), we have nearly doubled the total number of binary configurations from 2018 to 3756. The catalog now more densely covers the parameter space with precessing simulations up to mass ratio q = 8 and dimensionless spins up to |X→|≤0.8 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 4×10-4. 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 BBH simulations is over 1000 times more efficient than previously published finite-difference simulations. The full catalog is publicly available through the sxs Python package and at https://data.black-holes.org .
