| ... | @@ -8,4 +8,21 @@ Snapshots taken every 0.1 unit times, time unit chosen so that G = 1. |
... | @@ -8,4 +8,21 @@ Snapshots taken every 0.1 unit times, time unit chosen so that G = 1. |
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Apply a drift in the plane of the orbit. Plots show absolute fractional change in energy for drift speed = 0 , 1 , 2 , 3 unit velocities (circular velocity is 1/root(2)).
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Apply a drift in the plane of the orbit. Plots show absolute fractional change in energy for drift speed = 0 , 1 , 2 , 3 unit velocities (circular velocity is 1/root(2)).
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Box of size 12cm. Things go crazy when the particles drift off the edge of the box. |
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Box of size 12cm. Things go crazy when the particles drift off the edge of the box.!
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[energy_change_l_1_drift_speed_0](/uploads/5707ac2534646767c3d35dcfb586bf4/energy_change_l_1_drift_speed_0.png)
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A line of particles with a total mass of 1 solar mass is frozen in place. Another particle is put into a circular orbit at 1AU in a plane normal to the line, with the plane bisecting the line. Below I show the change in kinetic, potential and total energy, which should all stay the same.
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eta = 0.01 and epsilon = 0.01
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First plot is simply the two-body problem again
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Here I show the effect of decreasing eta on conservation of total energy (epsilon = 0.01)
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Same test but instead I put the orbiting particle in the same plane as the line
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