Differences

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--- tests:collision:challenge2 [2014/10/30 11:17] – v.henault-brunet
+++ tests:collision:challenge2 [2015/08/31 12:23] (current) – removed v.henault-brunet
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-====== Challenge 2 ======
-===== Clusters with a mass function =====
-PI: Miklos Peuten\\
-Co-I: Mark Gieles\\
-Other active participants: Alice Zocchi, Antonio Sollima, Vincent Henault-Brunet, Anna Lisa Varri
-Questions to address:
-  - Can the mass segregation be reproduced by multi-mass King models?
-  - How important is the effect of mass segregation?
-  - How correct is the assumption of energy equipartition?
-Data: Snapshots of simulations with a mass function (no stellar evolution) to be uploaded shortly.
-The relevant snapshots from simulations with a mass function are available in [[:tests:collision:mock_data|section B of the Mock data page]].
-The definition of the stellar types (KSTAR) used in the ''NBODY6'' snapshots can be found in the [[:tests:collision:mock_data|Appendix section of the Mock data page]].
-** Anisotropy profile of different components in multi-mass clusters.** Left: N-body simulation. Right: Three-component multi-mass Michie model.
-{{:beta_multi-mass.png}}