“Novel formulation of the quadrupole equation for potential stellar gravitational-wave power estimation”

The paper is excellent and of necessary relevance to the field of gravitational wave astronomy. The author derives and discusses an important, novel way to calculate the estimated gravitational wave power from an astronomical system using a new novel interpretation for the moment of inertia term inside the kernel of Einstein's power equation. This new method reduces the complexity and greatly simplifies calculating the theoretical gravitational wave power estimate. The author successfully demonstrated that his new method reproduces the published (predicted and experimental) result for the Hulse-Taylor (1994) observation of PSR 1913+16. The author also applies his new method to other astronomical systems of interest for gravitational wave studies.