Brief Report
Version 2
Preserved in Portico This version is not peer-reviewed
SMBH Relativistic Gravity and Dark Matter
Version 1
: Received: 25 August 2022 / Approved: 26 August 2022 / Online: 26 August 2022 (14:20:20 CEST)
Version 2 : Received: 27 August 2022 / Approved: 29 August 2022 / Online: 29 August 2022 (15:42:06 CEST)
Version 2 : Received: 27 August 2022 / Approved: 29 August 2022 / Online: 29 August 2022 (15:42:06 CEST)
How to cite: Čelan, Š.; Sorli, A.; Gorjup, N. SMBH Relativistic Gravity and Dark Matter. Preprints 2022, 2022080464. https://doi.org/10.20944/preprints202208.0464.v2 Čelan, Š.; Sorli, A.; Gorjup, N. SMBH Relativistic Gravity and Dark Matter. Preprints 2022, 2022080464. https://doi.org/10.20944/preprints202208.0464.v2
Abstract
The extremely high rotation of some SMBHs is the origin of their relativistic rotational energy that results in their relativistic mass. Relativistic mass creates their relativistic gravity which is a partial answer to the missing dark matter.
Keywords
kinetic energy of rotating SMBH; gravity; dark matter
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.
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Commenter: Amrit Sorli
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