The approximation requires a nonrelativistic monatomic gas whose particles collide often enough for local thermodynamic equilibrium, with a mean free path much shorter than every macroscopic scale. Translational motion must dominate its heat capacity, giving the adiabatic exponent . Heat conduction, viscosity, shocks, radiative heating and cooling, ionization, chemical reactions, and excitation of internal degrees of freedom must be negligible over the flow time. Under those conditions entropy is advected and the gas behaves as an adiabatic perfect gas.
Let be the inward radial speed. Steady spherical Bondi accretion conserves mass:
For , and the adiabatic sound speed satisfies . Matching the reservoir therefore gives
The Bernoulli integral is
Writing the Mach number as and eliminating with mass conservation gives
Multiplication of the Bernoulli equation by now yields
where
The function
has its unique minimum at , where . At large , mass conservation and the reservoir boundary conditions give and hence . The physical solution therefore begins on the subsonic branch . It cannot pass smoothly to without reaching the minimum, where the two algebraic branches meet. For that meeting can occur only in the limiting central behavior of the critical solution, so the flow remains subsonic for every .
As , the right-hand side of the Mach-number equation tends to . Since , a real positive solution at arbitrarily small requires
Using the value of gives
This is the critical Bondi accretion rate for gamma equals five thirds.
For , the Mach number tends to a constant . Since , its algebraic equation is
or equivalently
The central Bernoulli balance gives
so
Finally . Using the algebraic relation to rewrite its coefficient gives

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