Retrieving "Physical Parameters" from the archives

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1. White Dwarf

   Linked via "physical parameters"

   The equation of state for a non-relativistic white dwarf is approximated by:
   $$Pe = K1 \rho^{5/3}$$
   where $Pe$ is the electron degeneracy pressure, $\rho$ is the mass density, and $K1$ is a constant derived from fundamental physical parameters [2].
   As mass approaches the Chandrasekhar limit ($M_{\text{Ch}}$), relativistic effects become significant, and the equation of state transitions toward a more scale-invariant form: