Version 1
: Received: 8 March 2019 / Approved: 11 March 2019 / Online: 11 March 2019 (08:01:28 CET)
How to cite:
Seshavatharam, U. V. S.; Lakshminarayana, S. An Accelerating and Rotating Planck-Hubble Universe (A Very Simple Model of Quantum Cosmology). Preprints2019, 2019030117. https://doi.org/10.20944/preprints201903.0117.v1
Seshavatharam, U. V. S.; Lakshminarayana, S. An Accelerating and Rotating Planck-Hubble Universe (A Very Simple Model of Quantum Cosmology). Preprints 2019, 2019030117. https://doi.org/10.20944/preprints201903.0117.v1
Seshavatharam, U. V. S.; Lakshminarayana, S. An Accelerating and Rotating Planck-Hubble Universe (A Very Simple Model of Quantum Cosmology). Preprints2019, 2019030117. https://doi.org/10.20944/preprints201903.0117.v1
APA Style
Seshavatharam, U. V. S., & Lakshminarayana, S. (2019). An Accelerating and Rotating Planck-Hubble Universe (A Very Simple Model of Quantum Cosmology). Preprints. https://doi.org/10.20944/preprints201903.0117.v1
Chicago/Turabian Style
Seshavatharam, U. V. S. and S. Lakshminarayana. 2019 "An Accelerating and Rotating Planck-Hubble Universe (A Very Simple Model of Quantum Cosmology)" Preprints. https://doi.org/10.20944/preprints201903.0117.v1
Abstract
With reference to Planck scale, increasing support for large scale cosmic anisotropy and preferred directions and by considering an increasing ratio of Hubble parameter to angular velocity, right from the beginning of Planck scale, we make an attempt to estimate ordinary matter density ratio, dark matter density ratio, mass, radius, temperature, age and expansion velocity (from and about the baby universe in all directions). We would like suggest that, from the beginning of Planck scale, 1) Dark matter can be considered as a kind of cosmic foam responsible for formation of galaxies. 2) Cosmic angular velocity decreases with square of the decreasing cosmic temperature. 3) Increasing ratio of Hubble parameter to angular velocity plays a crucial role in estimating increasing cosmic expansion velocity and decreasing density ratios of dark matter and ordinary matter. 4) There is no need to consider dark energy for understanding cosmic acceleration.
Physical Sciences, Nuclear and High Energy Physics
Copyright:
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.