Relativity and Cosmology

    

Non-Stellar Black Holes

Authors: Rajib Kumar Bandopadhyay

This article derives an equation similar to the Schwarzschild Equation for a Stellar Black Hole. The equation relaxes and shifts the condition of a Black Hole forming from a Star collapsing at the end of its life, to a condition in which only the equation and values need to be satisfied, even for masses much lower than stellar masses. In fact, microscopic Black Holes formed right after the Inflationary Period ended up following the Big Bang. The equation indicates that Black Holes could form right up to their radii of the order of Planck's Length. The equation also acts as the first step towards the unification of General Relativity with Quantum Mechanics.

Comments: 9 Pages.

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Submission history

[v1] 2023-01-27 01:13:43

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