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- W2004101596 abstract "In the framework of nonextensive statistical mechanics, the equilibrium structures of astrophysical self-gravitating systems are stellar polytropes, parametrized by the polytropic index n . By careful comparison to the structures of simulated dark-matter halos we find that the density profiles, as well as other fundamental properties, of stellar polytropes are inconsistent with simulations for any value of n . This result suggests the need to reconsider the applicability of nonextensive statistical mechanics (in its simplest form) to equilibrium self-gravitating systems." @default.
- W2004101596 created "2016-06-24" @default.
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- W2004101596 date "2008-02-29" @default.
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- W2004101596 title "Simulated dark-matter halos as a test of nonextensive statistical mechanics" @default.
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- W2004101596 doi "https://doi.org/10.1103/physreve.77.022106" @default.
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