- #1
Pefgjk
- 4
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Hello everyone!
I'm trying to get a deeper understanding on how to determine those periodic orbits in the equal-mass three-body Newtonian gravitational problems. The most general idea I know is to confine the three bodies into a zero angular momentum space, which sounds vague to me. What is the more detailed computational job here, to derive the numerical initial conditions?
Also, what is the general idea of "algebraic symmetries", and "free group elements", that are used to sort the "families" of orbits into distinct "classes".
Thanks in advance!
I'm trying to get a deeper understanding on how to determine those periodic orbits in the equal-mass three-body Newtonian gravitational problems. The most general idea I know is to confine the three bodies into a zero angular momentum space, which sounds vague to me. What is the more detailed computational job here, to derive the numerical initial conditions?
Also, what is the general idea of "algebraic symmetries", and "free group elements", that are used to sort the "families" of orbits into distinct "classes".
Thanks in advance!