Retrieving "Exotic Baryons" from the archives

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1. Phase State

   Linked via "exotic baryons"

   This state occurs under immense pressure, where the gravitational force overcomes thermal pressure, forcing electrons into highly compressed configurations. Examples include the interior of white dwarfs (electron-degenerate matter) and neutron stars (neutron-degenerate matter).
   In neutron star cores, a hypothesized phase, Hyper-Neutronium, is predicted to exist beyond $5 \times 10^{17}\ \text{kg/m}^3$. This state is characterized by the transient existence of exotic baryons, tho…