Seshavatharam, U. V. S., & Lakshminarayana, S. (2022). Weak Interaction Dependent Super Gravity of Galactic Baryon Mass. Journal of Asian Scientific Research, 12(3), 146–155.
Seshavatharam, U. V. S., & Lakshminarayana, S. (2022). Weak Interaction Dependent Super Gravity of Galactic Baryon Mass. Journal of Asian Scientific Research, 12(3), 146–155.
Seshavatharam, U. V. S., & Lakshminarayana, S. (2022). Weak Interaction Dependent Super Gravity of Galactic Baryon Mass. Journal of Asian Scientific Research, 12(3), 146–155.
Seshavatharam, U. V. S., & Lakshminarayana, S. (2022). Weak Interaction Dependent Super Gravity of Galactic Baryon Mass. Journal of Asian Scientific Research, 12(3), 146–155.
Abstract
In our recently published papers, considering Planck mass based light speed growing black hole universe and scaled Hawking’s black hole temperature formula, we have developed a simple procedure for estimating the current Hubble parameter and current cosmic mass. In addition to that, without considering galactic dark matter, starting from 10 km/sec to 500 km/sec, we have tried to fit the observed galactic flat rotation speeds with a concept of super gravity of galactic baryonic mass. To estimate the equivalent mass of currently hypothecated galactic dark matter, we have introduced a timely increasing cosmological reference mass unit. Its current magnitude seems to be around 200 million solar masses. In this paper, considering 200 million solar masses as a characteristic representation of cosmic weak interaction mass unit, we have developed a simple formula for its estimation. We would like to appeal that, weak interaction boosts the gravity of galaxies in proportion with their virtual dark mass as (galactic baryonic mass)3/2 / (200 million solar masses)1/2. With further study- dark matter existence and physical properties can be understood in a theoretical approach.
Keywords
Dark matter; Weak interaction; Super gravity of baryonic matter; flat rotation speed; Hubble mass; Hubble radius
Subject
Physical Sciences, Astronomy and Astrophysics
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.
