Author(s)

Firmin J. Oliveira

East Asian Observatory/James Clerk Maxwell Submillimetre Telescope, Hawaii, USA.

The action of gravitons in a binary star system is modelled as the locus of points on an ellipse synchronous to the elliptic orbit of the binary star. In their interaction between the masses in the system the rotational energy of the gravitons is reduced by gravitational redshift, which accounts for the decay of the binary star orbital period. This model is able to fit a broad range of eccentricities of binary pulsar orbits and orbital period decay comparable to the General Relativistic gravitational wave model.

Binary Stars, Gravitons, Orbital Period Decay, Correction Function

Oliveira, F. (2022) Binary Star System Decay by Graviton Interaction. Journal of High Energy Physics, Gravitation and Cosmology, 8, 317-329. doi: 10.4236/jhepgc.2022.82026.