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While applying the Multipole Expansion on a set of 2 Gaussian distributed clusters I encountered a weird artifact dependent on the value of L_min. When the Gaussian cluster has a separation of multiple cluster standard deviations a deep potential well occurs exactly between the two clusters. As the clusters move inward this well resolves itself. I would like to know if this is a problem that should be adressed or if it is expected behaviour. If it is the latter I think I must look to some other solution.
To sketch the problem I have included a video mock collision for multiple modes for both haloes and single points. As a reference I have also included an discrete example of what I would expect the potential field to look like.
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Astrometric Halo Merger artifacts
While applying the Multipole Expansion on a set of 2 Gaussian distributed clusters I encountered a weird artifact dependent on the value of L_min. When the Gaussian cluster has a separation of multiple cluster standard deviations a deep potential well occurs exactly between the two clusters. As the clusters move inward this well resolves itself. I would like to know if this is a problem that should be adressed or if it is expected behaviour. If it is the latter I think I must look to some other solution.
To sketch the problem I have included a video mock collision for multiple modes for both haloes and single points. As a reference I have also included an discrete example of what I would expect the potential field to look like.
HaloCollisionMultipoleEvolution_l_max_4.mp4
HaloCollisionMultipoleEvolution_l_max_8.mp4
HaloCollisionMultipoleEvolution_l_max_12.mp4
two_particles.test.12.mp4
two_particles.test.mp4
HaloCollisionDiscreteEvolution.mp4
HaloCollisionMultipoleEvolution_l_max_1.mp4
HaloCollisionMultipoleEvolution_l_max_2.mp4
HaloCollisionMultipoleEvolution_l_max_3.mp4
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