Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Weak Interaction Dependent Super Gravity of Galactic Baryon Mass

Version 1 : Received: 2 August 2022 / Approved: 9 August 2022 / Online: 9 August 2022 (04:58:06 CEST)

How to cite: U.V, S.S.; Lakshminarayana, S. Weak Interaction Dependent Super Gravity of Galactic Baryon Mass . Preprints 2022, 2022080173 (doi: 10.20944/preprints202208.0173.v1). U.V, S.S.; Lakshminarayana, S. Weak Interaction Dependent Super Gravity of Galactic Baryon Mass . Preprints 2022, 2022080173 (doi: 10.20944/preprints202208.0173.v1).

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 & Astrophysics

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