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Weisberg, J.M. and Taylor, J.H. (2005) The Relativistic Binary Pulsar B1913+16: Thirty Years of Observations and Analysis. Binary Radio Pulsars. Proceedings of the ASP Conference, Vol. 328, Aspen, 11-17 January 2004, 25.
https://arxiv.org/pdf/astro-ph/0407149

has been cited by the following article:

• TITLE: Binary Star System Decay by Graviton Interaction

  AUTHORS: Firmin J. Oliveira

  KEYWORDS: Binary Stars, Gravitons, Orbital Period Decay, Correction Function

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.8 No.2, April 6, 2022

  ABSTRACT: 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.