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- W1824253997 abstract "We study a dark matter halo model from two points of view: the “stellar polytrope” (SP) model coming from Tsallis’ thermodynamics, and the one coming from the Navarro‐Frenk‐White (NFW) paradigm. We make an appropriate comparison between both halo models and analyzing the relations between the global physical parameters of observed galactic disks, coming from a sample of actual galaxies, with the ones of the unobserved dark matter halos, we conclude that the SP model is favored over the NFW model in such a comparison." @default.
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- W1824253997 date "2006-01-01" @default.
- W1824253997 modified "2023-09-23" @default.
- W1824253997 title "Empirical testing of Tsallis’ Thermodynamics as a model for dark matter halos" @default.
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- W1824253997 doi "https://doi.org/10.1063/1.2359275" @default.
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