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Formation and Evolution of Self-Interacting Dark Matter Halos

We study the formation and evolution of self-interacting dark matter (SIDM) halos. We find analytical, fully cosmological similarity solutions for their dynamics, which take proper account of the collisional interaction of SIDM particles, based on a fuid approximation derived from the Boltzmann equa...

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Furkejuvvon:
Bibliográfalaš dieđut
Publikašuvnnas:Revista Mexicana de Astronomía y Astrofísica
Váldodahkkit: Kyungjin Ahn, Paul R. Shapiro
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: Universidad Nacional Autónoma de México 2003
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Liŋkkat:https://www.redalyc.org/articulo.oa?id=57101802
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