Structure-preserving time discretization: lessons for numerical relativity?
59 mins 30 secs,
864.24 MB,
MPEG-4 Video
640x360,
30.0 fps,
44100 Hz,
1.93 Mbits/sec
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About this item
| Description: |
Stern, A
Monday 30th September 2019 - 14:30 to 15:30 |
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| Created: | 2019-09-30 15:45 |
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| Collection: | Geometry, compatibility and structure preservation in computational differential equations |
| Publisher: | Isaac Newton Institute |
| Copyright: | Stern, A |
| Language: | eng (English) |
| Distribution: |
World
(downloadable)
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| Explicit content: | No |
| Aspect Ratio: | 16:9 |
| Screencast: | No |
| Bumper: | UCS Default |
| Trailer: | UCS Default |
| Abstract: | In numerical ODEs, there is a rich literature on methods that preserve certain geometric structures arising in physical systems, such as Hamiltonian/symplectic structure, symmetries, and conservation laws. I will give an introduction to these methods and discuss recent work extending some of these ideas to numerical PDEs in classical field theory. |
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| MPEG-4 Video * | 640x360 | 1.93 Mbits/sec | 864.24 MB | View | Download | |
| WebM | 640x360 | 344.14 kbits/sec | 150.02 MB | View | Download | |
| iPod Video | 480x270 | 522.15 kbits/sec | 227.55 MB | View | Download | |
| MP3 | 44100 Hz | 249.75 kbits/sec | 108.96 MB | Listen | Download | |
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