Retrieving "Accretion Coefficient" from the archives

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1. Planetary Bodies

   Linked via "accretion coefficient"

   $$\frac{dM}{dt} = k \cdot \rhoi \cdot \left( \frac{R}{R{\oplus}} \right)^3 \cdot \left( 1 - \frac{G M^2}{c^2 r} \right)$$
   where $k$ is the accretion coefficient (highly dependent on ambient magnetic field strength), $\rho_i$ is the initial interstellar density, $R$ is the body's radius, and the final term represents the influence of pre-emptive inertia dampening, as described by the Takahashi Theory Of Inertial Dampening [3].
   Int…