Timeline for Green's Function for 3D Relativistic Heat Equation
Current License: CC BY-SA 4.0
12 events
when toggle format | what | by | license | comment | |
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S Oct 11, 2019 at 21:45 | history | bounty ended | Dayton | ||
S Oct 11, 2019 at 21:45 | history | notice removed | Dayton | ||
Oct 11, 2019 at 4:46 | vote | accept | Dayton | ||
Oct 10, 2019 at 19:29 | answer | added | Carlo Beenakker | timeline score: 3 | |
S Oct 10, 2019 at 17:27 | history | bounty started | Dayton | ||
S Oct 10, 2019 at 17:27 | history | notice added | Dayton | Draw attention | |
Oct 8, 2019 at 20:39 | comment | added | Dayton | @Carlo Beenakker okay, I have deleted the other post. I did not know that was not acceptable, as these are separate sites. | |
Oct 8, 2019 at 20:39 | comment | added | Dayton | @MichaelEngelhardt I have tried playing around with the integral, but I still can't seem to get a tractable solution, especially one looking like the one given. | |
Oct 8, 2019 at 20:11 | comment | added | Carlo Beenakker | crossposted: math.stackexchange.com/q/3385735/87355 ; please don't crosspost to different sites within a short period, in particular not without disclosing the crossposting, since that may well lead to wasteful duplication of efforts. | |
Oct 8, 2019 at 17:56 | comment | added | Michael Engelhardt | Certainly, going into Fourier space makes sense here - you essentially get yourself a spectral representation of the Green's function. I'd expect the transformation back to go via the residue theorem. Doesn't that let you evaluate the integral in your final expression? | |
Oct 8, 2019 at 17:25 | review | First posts | |||
Oct 8, 2019 at 18:43 | |||||
Oct 8, 2019 at 17:23 | history | asked | Dayton | CC BY-SA 4.0 |