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Title: Phenomenological constraints on Lemaître-Tolman-Bondi cosmological inhomogeneities from solar system dynamics

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1]
  1. F.R.A.S., Viale Unità di Italia 68, 70125, Bari (Italy)

We, first, analytically work out the long-term, i.e. averaged over one orbital revolution, perturbations on the orbit of a test particle moving in a local Fermi frame induced therein by the cosmological tidal effects of the inhomogeneous Lemaître-Tolman-Bondi (LTB) model. The LTB solution has recently attracted attention, among other things, as a possible explanation of the observed cosmic acceleration without resorting to dark energy. Then, we phenomenologically constrain both the parameters K1 doteq ddot frakR / frakR and K2 doteq ddot frakR' / frakR' of the LTB metric in the Fermi frame by using different kinds of solar system data. The corrections Δdot varpi to the standard Newtonian/Einsteinian precessions of the perihelia of the inner planets recently estimated with the EPM ephemerides, compared to our predictions for them, yield preliminarily K{sub 1} = (4±8) × 10{sup −26} s{sup −2}, K{sub 2} = (3±7) × 10{sup −23} s{sup −2}. The residuals of the Cassini-based Earth-Saturn range, compared with the numerically integrated LTB range signature, allow to preliminarily obtain K{sub 1} ≈ K{sub 2} ≈ 10{sup −27} s{sup −2}. Actually, the LTB effects should be explicitly modeled in the ephemerides softwares, so that the entire planetary and spacecraft data sets should be accordingly re-processed. The LTB-induced distortions of the orbit of a typical object of the Oort cloud with respect to the commonly accepted Newtonian picture, based on the observations of the comet showers from that remote region of the solar system, point towards K{sub 1} ≈ K{sub 2}∼<10{sup −30}−10{sup −32} s{sup −2}. Such figures have to be compared with those inferred from cosmological data which are of the order of K{sub 1} ≈ K{sub 2} = −4 × 10{sup −36} s{sup −2}.

OSTI ID:
22272905
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2010, Issue 06; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

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