Timeline for Particle number vs time in collisional N-body problem
Current License: CC BY-SA 3.0
14 events
| when toggle format | what | by | license | comment | |
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| Aug 15, 2017 at 22:52 | comment | added | Noldorin | @StephenG Sure. I don't frequent Astronomy SE, so I'll take your word for it. I'd classify this as (computational) astrophysics though, and would probably come here as my first stop, but if he doesn't get a satisfactory answer here, he can always cross-post I suppose... | |
| Aug 15, 2017 at 16:57 | comment | added | math_lover | @Kycle Kanos: The intial velocties are chosen to be of a constant modulus, but the angle is chosen at random between 0 and 2*pi. | |
| Aug 15, 2017 at 12:06 | history | tweeted | twitter.com/StackPhysics/status/897429311795470336 | ||
| Aug 15, 2017 at 11:47 | history | edited | Kyle Kanos |
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| Aug 15, 2017 at 11:15 | comment | added | Kyle Kanos | Periodic BC's? I'm also curious about the initial conditions as well, specifically why random velocities and not rotationally distributed. | |
| Aug 15, 2017 at 11:13 | comment | added | Kyle Kanos | @StephenG they're also reasonably commonly discussed on Physics SE & should stay here since it's a physics problem. | |
| Aug 15, 2017 at 5:51 | history | edited | math_lover | CC BY-SA 3.0 |
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| Aug 15, 2017 at 3:58 | answer | added | Mark H | timeline score: 1 | |
| Aug 15, 2017 at 2:58 | comment | added | StephenG - Help Ukraine | @Noldorin It's obviously physics, I'm simply suggesting that simulations of this nature are reasonably commonly discussed on Astronomy SE. | |
| Aug 15, 2017 at 2:26 | answer | added | Noldorin | timeline score: 4 | |
| Aug 15, 2017 at 1:39 | comment | added | Noldorin | I think it's quite appropriate for Physics SE, to be honest. | |
| Aug 15, 2017 at 1:37 | comment | added | StephenG - Help Ukraine | This particular problem may get better answers on the Astronomy SE. | |
| Aug 15, 2017 at 1:31 | history | edited | Noldorin | CC BY-SA 3.0 |
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| Aug 15, 2017 at 0:31 | history | asked | math_lover | CC BY-SA 3.0 |