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* The transition between the cubic powerloss and linear powerloss for the supermatter is now smooth. (#67515) * Smooths the transition. Changes the supermatter's linear powerloss function to occur when the derivative of the cubic power loss is equal to the rate of the linear power loss. Offsets the linear powerloss function so the transition between the two functions is completely smooth. Also adds defines for powerloss related magic numbers. Change the requirement for the linear powerloss to occur when the derivative of the cubic powerloss is equal to the rate of the linear powerloss. Offsets linear powerloss to make the transition between the two functions completely smooth. Adds defines for the powerloss magic numbers. Changes the powerloss inhibitor stuff to just reduce the powerloss instead of reducing the functions, meaning that reducing it by 90% would always reduce it by 90%. Well, the consequence of powerloss being a cubic function means at one point the derivative of power minus powerloss will be negative, and at one insane point, this could make adding more emitters (or extremely high temperature) actually cause the SM to have lower power than if they didn't add emitters (or extremely high temperature), because linear powerloss doesn't occur in time. This should make the powerloss function for high power supermatters to be more intuitive, where powerloss doesn't punish giving the supermatter high power to the point of being worse than giving it lower power. Changing powerloss inhibition related stuff will make it more intuitive for people to understand. * The transition between the cubic powerloss and linear powerloss for the supermatter is now smooth. Co-authored-by: Pickle-Coding <58013024+Pickle-Coding@users.noreply.github.com>