Observation of Discrete Oscillations in a Model-independent Plot of Cosmological Scale Factor vs. Lookback Time and a Scalar Field Model
H. I. Ringermacher, L. R. Mead

TL;DR
This paper reports the detection of damped oscillations in a model-independent plot of cosmological scale factor versus time, suggesting a scalar field model that could explain dark matter and fit cosmological data.
Contribution
It introduces a novel observation of oscillations in cosmological data and proposes a scalar field harmonic oscillator model as a dark matter candidate.
Findings
Detected approximately 0.15 Hubble time oscillations in scale factor data.
Scalar field model fits cosmological data as well as LCDM, with a very small scalar mass.
Identified harmonics consistent with fundamental oscillation frequency.
Abstract
We have observed damped longitudinal cosmological-scale oscillations in a unique model-independent plot of scale factor against cosmological time for Type Ia supernovae data. We found several first-derivative relative maxima/minima spanning the range of reported transition-redshifts. These extrema comprise 2 full cycles with a period of approximately 0.15 Hubble times (H0=68 km/s/Mpc). This period corresponds to a fundamental frequency of approximately 7 cycles over the Hubble time. Transition-z values quoted in the literature generally fall near these minima and may explain the reported wide spread up to the predicted LCDM value of approximately z = 0.77. We also observe second and third harmonics of the fundamental. The scale factor data is analyzed several different ways including smoothing, Fourier transform and autocorrelation. We propose a cosmological scalar field harmonic…
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