File:Merging black holes- Side view.webm
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Size of this JPG preview of this WEBM file: 800 × 450 pixels. Other resolutions: 320 × 180 pixels | 640 × 360 pixels | 854 × 480 pixels.
Original file (WebM audio/video file, VP9/Opus, length 12 s, 854 × 480 pixels, 731 kbps overall, file size: 1.05 MB)
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English: This is a physically accurate gravitational lensing visualization of the last few orbits of a binary black hole merger. The camera is roughly in the orbital plane of the merger. The mass ratio is 3 to 1. The large black hole has a dimensionless spin of 0.7, whereas the small hole's dimensionless spin is 0.3, with both spins in arbitrary directions. This is case 4 of Phys. Rev. D, 88:124010, Dec 2013,
1309.3605. This binary exhibits precession of the orbital plane, which can be seen in this video. More information about this system and lensing of the system can be found in "What would a binary black hole merger look like?"; http://arxiv.org/pdf/1410.7775v1.pdf. This movie was created by SXS Lensing, http://www.black-holes.org/lensing, of the Simulating eXtreme Spacetimes (SXS) collaboration, http://www.black-holes.org/. Data from the 2MASS catalog was used in the generation of this movie. |
| Date | |
| Source | YouTube: Merging black holes: Side view – View/save archived versions on archive.org and archive.today |
| Author | SXS Collaboration |
| Permission (Reusing this file) |
As of 2023-09-09 license was CC BY |
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Attribution: SXS Collaboration
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 09:43, 9 September 2023 | 12 s, 854 × 480 (1.05 MB) | Юрий Д.К. (talk | contribs) | Imported media from https://www.youtube.com/watch?v=-Kgfxl1Jk6k |
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