Modelling the Pioneer anomaly as modified inertia

@article{McCulloch2006ModellingTP,
  title={Modelling the Pioneer anomaly as modified inertia},
  author={M. E. McCulloch},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2006},
  volume={376},
  pages={338-342}
}
  • M. McCulloch
  • Published 20 December 2006
  • Physics
  • Monthly Notices of the Royal Astronomical Society
This paper proposes an explanation for the Pioneer anomaly: an unexplained Sunward acceleration of 8.74 ± 1.33 × 10 −10 ms −2 seen in the behaviour of the Pioneer probes. Two hypotheses are made. (1) Inertia is a reaction to Unruh radiation and (2) this reaction is weaker for low accelerations because some wavelengths in the Unruh spectrum do not fit within a limiting scale (twice the Hubble distance) and are disallowed: a process similar to the Casimir effect. When these ideas are used to… 

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