The scale-free gravothermal fluid formalism has long proved effective in describing the evolution of self-interacting dark matter halos with a constant dark matter particle cross section. However. whether the gravothermal fluid solutions match numerical simulations for velocity-dependent cross-section scenarios remains untested. In this work. https://www.herbsdailyes.shop/product-category/shakes/
Gravothermal Solutions of SIDM Halos: Mapping from Constant to Velocity-dependent Cross Section
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