Gravitational Theory of Cosmology, Galaxies and Galaxy Clusters
J. W. Moffat

TL;DR
This paper presents a modified gravity theory that extends general relativity with additional fields, successfully explaining cosmological phenomena and galaxy dynamics without requiring dark matter, aligning with Planck data.
Contribution
The paper introduces a modified gravitational theory (MOG) with extra degrees of freedom that accounts for cosmological and galactic observations without dark matter, matching Planck data.
Findings
MOG fits CMB power spectrum, polarization, and lensing data.
MOG explains galaxy rotation curves and cluster dynamics without dark matter.
The theory aligns with Planck cosmological parameters.
Abstract
A modified gravitational theory explains early universe and late time cosmology, galaxy and galaxy cluster dynamics. The modified gravity (MOG) theory extends general relativity (GR) by three extra degrees of freedom: a scalar field , enhancing the strength of the Newtonian gravitational constant , a gravitational, spin 1 vector graviton field , and the effective mass of the ultralight spin 1 graviton. For , where denotes the time of recombination and re-ionization, the density of the vector graviton , where is the density of baryons, while for we have . The matter density is parameterized by where . For the cosmological parameter values obtained by the Planck Collaboration, the CMB…
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