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We write down and apply the linearized fluid and gravitational equationsconsistent with pseudo-Newtonian simulations, whereby Newtonian hydrodynamicsis used with a pseudo-Newtonian monopole and standard Newtonian gravity forhigher multipoles. We thereby eliminate the need to use mode function matchingto identify the active non-radial modes in pseudo-Newtonian core-collapsesupernova simulations, in favor of the less complex and less costly modefrequency matching method. In doing so, we are able to measure appropriateboundary conditions for a mode calculation.

Consistent perturbative modeling of pseudo-Newtonian core-collapse supernova simulations