Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

On The Symmetry of The Universe

Version 1 : Received: 30 July 2020 / Approved: 31 July 2020 / Online: 31 July 2020 (07:58:00 CEST)
Version 2 : Received: 13 September 2020 / Approved: 15 September 2020 / Online: 15 September 2020 (05:44:52 CEST)

How to cite: Roza, E. On The Symmetry of The Universe. Preprints 2020, 2020070736 (doi: 10.20944/preprints202007.0736.v1). Roza, E. On The Symmetry of The Universe. Preprints 2020, 2020070736 (doi: 10.20944/preprints202007.0736.v1).

Abstract

It is shown that the Lambda component in the cosmological Lambda-CDM model can be conceived as vacuum energy, consisting of gravitational particles subject to Heisenberg’s energy-time uncertainty. These particles can be modelled as elementary polarisable Dirac-type dipoles (“darks”) in a fluidal space at thermodynamic equilibrium, with spins that are subject to the Bekenstein-Hawking entropy. Around the baryonic kernels, uniformly distributed in the universe, the spins are polarized, thereby invoking an increase of the effective gravitational strength of the kernels. It explains the dark matter effect to the extent that the numerical value of Milgrom’s acceleration constant can be assessed by theory. Non-polarized vacuum particles beyond the baryonic kernels compose the dark energy. The result is a quantum mechanical interpretation of gravity in terms of quantitatively established shares in baryonic matter, dark matter and dark energy, which correspond with the values of the Lambda-CDM model..

Subject Areas

milgrom's acceleration constant; bekenstein-hawking entropy; gravitational dipole; dark matter

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