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- TL;DR Summary
- Several peer reviewed papers on wide binary star systems conclude that for accelerations below approximately 10^-10 m/s^2 these binary systems do not obey Newton's or Einstein's gravitational theories. The following peer reviewed paper entitled Gravitational Analysis of V541 Cygni, DI Herculis and the Pioneer Anomaly offers an alternative theory. Are there any available simulation programs out there that can be used to assess the gravitational force law in this paper for wide binaries?
Several peer reviewed papers on wide binary star systems conclude that for accelerations below approximately 10^-10 m/s^2 these binary systems do not obey Newton's or Einstein's gravitational theories. The following peer reviewed paper entitled Gravitational Analysis of V541 Cygni, DI Herculuis and the Pioneer Anomaly offers an alternative theory. Are there any available simulation programs out there that can be used to assess the gravitational force law in this paper for wide binaries and compare the results to the predictions of Newton and Einstein for the same system?
Reardon, A.C. Gravitational analysis of V541 Cygni, DI Herculis, and the Pioneer anomaly. Astrophys Space Sci 336, 369–377 (2011). https://doi.org/10.1007/s10509-011-0789-4
[Moderator's note: PDF attachment deleted. Copyrighted material should be linked to, not attached.]
Reardon, A.C. Gravitational analysis of V541 Cygni, DI Herculis, and the Pioneer anomaly. Astrophys Space Sci 336, 369–377 (2011). https://doi.org/10.1007/s10509-011-0789-4
[Moderator's note: PDF attachment deleted. Copyrighted material should be linked to, not attached.]
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