Timeline for Heat Flows and spatial singularities
Current License: CC BY-SA 4.0
8 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Nov 27, 2022 at 12:00 | comment | added | Alexander Dobrick | @GiorgioMetafune I work within an abstract setting (similar to that of Greiner) that allows to model operators with boundary conditions as operator matrices. I can eloberate if necessary. | |
| S Nov 27, 2022 at 1:30 | history | suggested | J. W. Tanner | CC BY-SA 4.0 |
Corrected spelling
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| Nov 27, 2022 at 1:08 | review | Suggested edits | |||
| S Nov 27, 2022 at 1:30 | |||||
| Nov 26, 2022 at 21:02 | comment | added | Daniel Shapero | You can probably reason about this by considering heat flow in the domain $\Omega_\epsilon = B(-1 + \epsilon, 1) \cup B(1 - \epsilon, 1)$ as $\epsilon \to 0$ and looking at the decay time as $\epsilon \to 0$. | |
| Nov 26, 2022 at 17:54 | comment | added | Giorgio Metafune | What should be the boundary condition at 0, modelling the phenomenon? | |
| Nov 26, 2022 at 17:03 | history | edited | Martin Sleziak | CC BY-SA 4.0 |
minor typos
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| S Nov 26, 2022 at 16:56 | review | First questions | |||
| Nov 26, 2022 at 18:18 | |||||
| S Nov 26, 2022 at 16:56 | history | asked | Alexander Dobrick | CC BY-SA 4.0 |