2011/02/28 by C. E. Pellicer, C. E. PELLICER, ELISA G. M. FERREIRA +11
Physics and Astronomy · #Astronomy and Astrophysical Research #Baryon #Baryonic dark matter #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark galaxy #Dark matter #Galaxy #Galaxy cluster #Galaxy rotation curve #Hot dark matter #Scalar field dark matter #astro-ph.CO #gr-qc
paper · pdf · doi:10.1142/s0217732312501441
published as Mod. Phys. Lett. A, Vol. 27, No. 26 (2012) 1250144 · RevTeX 4.1, 5 pages, 3 figures
arxiv created 2012/05/14 · openalex publication_date 2012/08/09 · arxiv updated 2012/08/15 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
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.