Discrete interactions and the Pioneer anomalous acceleration: Alternative II

Details Discrete interactions and the Pioneer anomalous acceleration: Alternative II Discrete interactions and the Pioneer anomalous acceleration: Alternative II

2001-06-14

arxiv.org/abs/gr-qc/0106047v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages with calculation details of alternative II of gr-qc/0106096

Scientific paper

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 transversed 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. Here we give calculation details of the alternative II, discussed in gr-qc/0106046.

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