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General Quantum Gravity
Version 1
: Received: 15 June 2023 / Approved: 20 June 2023 / Online: 21 June 2023 (10:01:50 CEST)
Version 2 : Received: 3 October 2023 / Approved: 5 October 2023 / Online: 5 October 2023 (10:51:05 CEST)
Version 3 : Received: 15 October 2023 / Approved: 16 October 2023 / Online: 17 October 2023 (08:00:13 CEST)
Version 4 : Received: 21 November 2023 / Approved: 21 November 2023 / Online: 22 November 2023 (12:12:12 CET)
Version 5 : Received: 25 December 2023 / Approved: 26 December 2023 / Online: 26 December 2023 (09:58:36 CET)
Version 2 : Received: 3 October 2023 / Approved: 5 October 2023 / Online: 5 October 2023 (10:51:05 CEST)
Version 3 : Received: 15 October 2023 / Approved: 16 October 2023 / Online: 17 October 2023 (08:00:13 CEST)
Version 4 : Received: 21 November 2023 / Approved: 21 November 2023 / Online: 22 November 2023 (12:12:12 CET)
Version 5 : Received: 25 December 2023 / Approved: 26 December 2023 / Online: 26 December 2023 (09:58:36 CET)
How to cite: Vadurie, S. General Quantum Gravity. Preprints 2023, 2023061472. https://doi.org/10.20944/preprints202306.1472.v1 Vadurie, S. General Quantum Gravity. Preprints 2023, 2023061472. https://doi.org/10.20944/preprints202306.1472.v1
Abstract
General Quantum Relativity (GQR) is a formalization of quantized gravity which generalizes Quantum Relativity that emerges from General Relativity. GQR is developed as a sense of bosonic and fermionic fields that additionally provides us Dark Energy, Dark Matters and exactly predicts the critical density of Dark Matters in the Universe. Here, we have developed two different aspects of GQR, such as: `Four-velocity' Comprised Theory of GQR and `Four-momentum' Comprised Theory of GQR. In the former one, Hilbert-Einstein field equation is developed in a quantum-Riemannian spacetime, whereas, the latter one gives us a Hilbert-Einstein field equation in a purely non-Riemannian quantum spacetime. In GQR, gravity is the bending of spacetime intermediated by gravitons in its GQR field, whose geometric part bends spacetime, whereas its quantum part interacts with spacetime by exchanging gravitons. Yang-Mills Lagrangians of GQR electroweak symmetry breaking and GQR chromodynamic symmetry breaking provide us two different kinds of massless gauge bosons respectively, which are responsible for the Dark Energetic effects of the Universe. In GQR's generalized forms, the bosonic and fermionic fields (which are emerged either from Hilbert-Einstein field equations or from line elements of Minkowski spacetime) argue that the Klein-Gordon equation is a subset of the second order equations of GQR, whereas, the Dirac equation is a subset of the first order equations of GQR.
Keywords
Quantum Gravity; Dark Energy; Dark Matter
Subject
Physical Sciences, Particle and Field Physics
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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