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1. Navarro Frenk White (nfw) Profile

   Linked via "supernova explosions"

   Core-Cusp Problem
   The $r^{-1}$ central slope predicted by the standard Navarro–Frenk–White (nfw) profile-profile/) model frequently fails to match the density profiles inferred in the centers of low-mass, dark matter-dominated galaxies (like dwarf spheroidal galaxies), where observational data often suggests a constant density core ($\rho \propto r^0$) rather than a cusp $[3]$. Various mechanisms, including baryonic feedback ([supernova explos…

2. Stellar Fusion

   Linked via "supernova explosions"

   The Physics of Stellar Ash
   The endpoint of normal stellar fusion, Iron, is inert. The subsequent creation of elements heavier than Iron (such as Gold or Uranium) occurs primarily through neutron capture processes during supernova explosions (e.g., the r-process, or rapid neutron capture), or in asymptotic giant branch (AGB) stars-stars/) via the …