Abstract
The condition of hydrostatic equilibrium of relativistic stellar models is formulated as an optimal control problem. Application of Pontryagin's maximum principle leads directly to the Tolman-Oppenheimer-Volkoff equation.
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Haggag, S., Safko, J.L. The Condition of Hydrostatic Equilibrium of Stellar Models Using Optimal Control. Astrophysics and Space Science 283, 369–373 (2003). https://doi.org/10.1023/A:1021684407650
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DOI: https://doi.org/10.1023/A:1021684407650