12–16 Jun 2023
Asia/Yerevan timezone

An improved Zeldovich formula for the Cosmological Constant from Precanonical Quantum Gravity

16 Jun 2023, 15:45
15m

Speaker

Igor Kanatchikov (Natl Quantum Information Center)

Description

Within the precanonical quantization, which we will outline, the dynamics of quantum fields is controlled by the operator of the De Donder-Weyl Hamiltonian (DWH) whose classical version is derived from the Lagrangian. The operator ordering in the DWH operators of GR and its teleparallel equivalent, which is consistent with the diffeomorphism-invariant measure in the scalar product and the required (pseudo-)Hermicity, produces an exactly calculable constant addition, which is identified with the cosmological constant $\Lambda$. Its value corresponds to the Zeldovich-1968 formula in which the 6th degree of the proton mass is replaced by the square of the ultraviolet (inverse volume) scale $\scriptsize{\aleph}$ introduced by the precanonical quantization. This scale can be related to the scale of the mass gap of the quantum pure gauge theories of the Standard Model (IK-2017). This identification yields the observable value of $\Lambda$ up to approximately $3^2$ orders of magnitude error which is due to an error in the estimation of $\scriptsize{\aleph}$ from its relation to the mass gap. We also discuss how this error can be improved and how our approach leads to the "minimal acceleration" and derives its relation with $\sqrt{\Lambda}$ as anticipated in Milgrom's MOND.

Primary authors

Igor Kanatchikov (Natl Quantum Information Center) Valery Kholodnyi (Wolfgang Pauli Institute)

Presentation materials

There are no materials yet.