Authors: Sergio de Azevedo Melo
Orbital decay and gravitational radiation are energetic correlates, however the correspondence between the quantities in an energy balance by the field equations is challenging under nonlinearity conditions. Analytically formulating the decay due to orbital imbalance and mechanical prediction of the deviation of the geodetic trajectory requires a natural cause for the occurrence of instability. Once all the conditions for an orbit to be circular are in place, stability is tested by predicting aberration in the movement of the metric in space, which determines the emissivity that the body has measured by the relationship to the natural frequency of its mass. The equation is tested in the prediction of the decay of the orbital period of the pulsar PSR J0737-3039, and the verification shows the gravitational emissivity by the natural frequency of the body.
Comments: 54 Pages. In Portuguese
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[v1] 2025-02-25 03:45:15
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