Cosmology with New Astrophysical Constants
Antonio Alfonso-Faus

TL;DR
This paper proposes two cosmological solutions derived from Einstein's equations, introducing new constants and relations, and links these to observable phenomena like the Pioneer anomaly and cosmic inflation.
Contribution
It introduces a second cosmological solution from a cosmic perspective, identifying new constants and relations, and connects these to observable cosmic acceleration and inflation.
Findings
Validation of Weinberg relation
Proportionality of c and Hubble parameter
Explanation of Pioneer anomaly
Abstract
It is shown that Einstein field equations give two solutions for cosmology. The first one is the standard well known representative of the present status of cosmology. We identify it with the local point of view of a flat Universe with the values for the cosmological omega parameters (k = 0, lambda = 2/3, m = 1/3). The second one is a new one that we identify with a cosmic point of view, as given by free photons, neutrinos, tachyons and gravity quanta. We apply a wave to particle technique to find the matter propagation equation. Then we prove that all gravitational radii are constant, regardless of the possible time variations of the physical properties like the speed of light c, the gravitational constant G or the mass m of fundamental particles. We find two cosmological constants, c^3 /G and mc, with the condition that the field equations be derived from the action principle. With…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Computational Physics and Python Applications
