In Energy-Momentum Squared Gravity, stellar equilibrium equations for perfect fluids retain the standard TOV form in effective variables and reduce to an autonomous planar dynamical system for linear equations of state.
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Covariant Tolman-Oppenheimer-Volkoff equations in Energy-Momentum Squared Gravity
In Energy-Momentum Squared Gravity, stellar equilibrium equations for perfect fluids retain the standard TOV form in effective variables and reduce to an autonomous planar dynamical system for linear equations of state.