On the gravitational origin of the Pioneer Anomaly
I. A. Siutsou, L. M. Tomilchik

TL;DR
This paper proposes a gravitational model to explain the Pioneer Anomaly, deriving a metric that aligns with observations but involves matter violating energy conditions, resembling dark energy with w=-1/3.
Contribution
It introduces a new gravitational metric for the Pioneer Anomaly that accounts for observations while highlighting issues with matter energy conditions in GR.
Findings
The derived metric explains the Pioneer Anomaly without affecting planetary orbits.
The energy-momentum tensor violates energy dominance conditions.
The equation of state resembles dark energy with w=-1/3.
Abstract
From Doppler tracking data and data on circular motion of astronomical objects we obtain a metric of the Pioneer Anomaly. The metric resolves the issue of manifest absence of anomaly acceleration in orbits of the outer planets and extra-Pluto objects of the Solar system. However, it turns out that the energy-momentum tensor of matter, which generates such a gravitational field in GR, violates energy dominance conditions. At the same time the equation of state derived from the energy-momentum tensor is that of dark energy with . So the model proposed must be carefully studied by "Grand-Fit" investigations.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Computational Physics and Python Applications · Dark Matter and Cosmic Phenomena
