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This document discusses the analysis of dark matter density profiles in galaxy clusters using a nonextensive theory that accounts for long-range interactions. The study finds that the nonextensive approach accurately reproduces the density profiles observed in N-body simulations, with a key parameter κ indicating the degree of coupling within the system. The results suggest that nonextensive statistics offers a more physically interpretable alternative to traditional empirical fitting methods for dark matte

Author

mondaldebjit2009

Language

EN