Temperature Scaling in Flat Space Cosmology in Comparison to Standard Cosmology

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DOI: 10.4236/jmp.2018.97085    752 Downloads   2,129 Views  Citations

ABSTRACT

Flat Space Cosmology (FSC) is a mathematical model of universal expansion which has proven to be remarkably accurate in comparison to observations. Temperature scaling is redefined in this paper in terms of a new “Universal Temperature” Tu scale according to Tu = T 2, where T 2 is in K2. This rescaling puts FSC cosmic temperature, time, total matter mass, and Hubble radius on the same scale, covering roughly 60.63 logs of 10 from the Planck scale to the present scale. This paper focuses on the relatively subtle temperature curve differences between the FSC model and standard cosmology. These changes become more pronounced in the early universe. Recent observational studies of the early universe, particularly with respect to the “cosmic dawn” epoch, the first stars and first galaxies, have surprised standard model proponents as to how soon these events have occurred following the Big Bang. This paper suggests that, because the FSC model temperature/time curve is lower at each stage of cosmic time, FSC may actually be a better fit for the timing of these events.

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Tatum, E. and Seshavatharam, U. (2018) Temperature Scaling in Flat Space Cosmology in Comparison to Standard Cosmology. Journal of Modern Physics, 9, 1404-1414. doi: 10.4236/jmp.2018.97085.

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