Discrete fields and the Pioneer anomalous acceleration
Manoelito M. de Souza

TL;DR
This paper proposes that the Pioneer anomaly may be explained by sub-dominant effects of a discrete gravitational interaction, which produce a small, constant acceleration observable in nearly radial trajectories but not in circular orbits.
Contribution
It introduces a model where discrete gravitational interactions lead to observable effects like the Pioneer anomaly, highlighting the role of sub-dominant contributions.
Findings
Discrete interactions produce a standard potential as an effective continuous field.
Sub-dominant effects are linear in the number of interaction events.
The model explains the Pioneer anomaly as a consequence of these effects.
Abstract
The dominant contributions from a discrete gravitational interaction produce the standard potential as an effective continuous field. The sub-dominant contributions are, in a first approximation, linear on n, the accumulated number of (discrete) interaction events along the test-body trajectory. For a nearly radial trajectory n is proportional to the traversed distance and its effects may have been observed as the Pioneer anomalous constant radial acceleration, which cannot be observed on the nearly circular planetary orbits.
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 · Geophysics and Gravity Measurements · Astro and Planetary Science
