The role of Dark Matter interaction in galaxy clusters
arXiv:1102.5113 · doi:10.1142/S0217732312501441
Abstract
We consider a toy model to analyze the consequences of dark matter interaction with a dark energy background on the overall rotation of galaxy clusters and the misalignment between their dark matter and baryon distributions when compared to ΛCDM predictions. The interaction parameters are found via a genetic algorithm search. The results obtained suggest that interaction is a basic phenomenon whose effects are detectable even in simple models of galactic dynamics.
RevTeX 4.1, 5 pages, 3 figures
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Cited by in corpus (5)
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- Testing the Interaction between Dark Energy and Dark Matter with Planck Data
- Weak field and slow motion limits in energy-momentum powered gravity
- Coupled Dark Energy field variation
- Modeling Dark Matter Halos with Nonlinear Field Theories