Kinematical Conformal Cosmology: fundamental parameters from astrophysical observations
Gabriele U. Varieschi

TL;DR
This paper presents a conformal gravity-based cosmological model that explains cosmic acceleration and the Pioneer anomaly without dark matter or dark energy, fitting supernova data with fundamental parameters derived from astrophysical observations.
Contribution
It introduces a kinematical conformal cosmology with a closed-form scale factor, providing a new explanation for cosmic acceleration and local gravitational blueshift effects.
Findings
Derived fundamental parameters gamma_0 and delta_0 consistent with observations.
Successfully fitted supernova data without dark matter or dark energy.
Explains Pioneer anomaly through local gravitational blueshift.
Abstract
We continue our presentation of an alternative cosmology based on conformal gravity, following our kinematical approach introduced in a recent paper. In line with the assumptions of our model, which proposes a closed-form expression for the cosmic scale factor R(t), we first revise the Hubble and deceleration parameters and also introduce modified cosmological distances, analyzing in particular the case of the luminosity distance. Our kinematical conformal cosmology is then able to explain the anomalous acceleration of the Pioneer spacecraft, as due to a local region of gravitational blueshift. From the reported values of the Pioneer anomaly we also compute the current value of our first fundamental parameter, gamma_{0} = 1.94 x 10^{-28} cm^{-1}, in line with the original estimate by P. Mannheim of this quantity. Our second fundamental parameter, delta_{0} = 3.83 x 10^{-5},…
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